cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Previous Archaeological Investigations at The Hotel Site (8BR240)
Creators: name: Gibbons, Rebecca
Year: 2018
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Hotel Site
valueUri: https://core.tdar.org/browse/site-name/116782/hotel-site
subject: 8BR00240
valueUri: https://core.tdar.org/browse/site-name/116103/8br00240
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Archaeological Overview
valueUri: https://core.tdar.org/browse/investigation-type/1/archaeological-overview
subject: Historic Background Research
valueUri: https://core.tdar.org/browse/investigation-type/18/historic-background-research
subject: Methodology, Theory, or Synthesis
valueUri: https://core.tdar.org/browse/investigation-type/6/methodology-theory-or-synthesis
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: The paper reviews the previous investigations conducted at the Hotel Site (8BR240) while focusing on the past archaeological surveys and historical analyses.
The Focusing Optics X-ray Solar Imager (FOXSI)
Creators: name: Christe, Steven
name: Alaoui, Meriem
name: Allred, Joel
name: Battaglia, Marina
name: Baumgartner, Wayne
name: Buitrago-Casas, Juan Camilo
name: Caspi, Amir
name: Chen, Bin
name: Chen, Thomas
name: Dennis, Brian
name: Drake, James
name: Glesener, Lindsay
name: Hannah, Iain
name: Hayes, Laura A.
name: Hudson, Hugh
name: Inglis, Andrew
name: Ireland, Jack
name: Klimchuk, James
name: Kowalski, Adam
name: Krucker, Säm
name: Massone, Anna Maria
name: Musset, Sophie
name: Piana, Michele
name: Ryan, Daniel
name: Shih, Albert Y.
name: Veronig, Astrid
name: Vilmer, Nicole
name: Warmuth, Alexander
name: White, Stephen
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: FOXSI is a direct-imaging, hard X-ray (HXR) telescope optimized for solar flare observations. It detects hot plasma and energetic electrons in and near energy release sites in the solar corona via bremsstrahlung emission, measuring both spatial structure and particle energy distributions. It provides two orders of magnitude faster imaging spectroscopy than previously available, probing physically relevant timescales (<1s) never before accessible to address fundamental questions of energy release and efficient particle acceleration that have importance far beyond their solar application (e.g., planetary magnetospheres, flaring stars, accretion disks). FOXSI measures not only the bright chromospheric X-ray emission where electrons lose most of their energy, but also simultaneous emission from electrons as they are accelerated in the corona and propagate along magnetic field lines. FOXSI detects emission from high in the tenuous corona, where previous instruments have been blinded by nearby bright features and will fully characterizes the accelerated electrons and hottest plasmas as they evolve in energy, space, and time to solve the mystery of how impulsive energy release leads to solar eruptions, the primary drivers of space weather at Earth, and how those eruptions are energized and evolve.
description: White paper submitted to the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033; 14 pages, 4 figures, 1 table
Потребление углеводсодержащих напитков и их вклад в общую калорийность рациона
Creators: name: Ханферьян Р.А.
name: Раджабкадиев Р.М.
name: Евстратова В.С.
name: Галстян А.Г.
name: Хуршудян С.А.
name: Сёмин В.Б.
name: Вржесинская О.А.
name: Акимов М.Ю.
Publisher: name: Вопросы питания
Year: 2018
Subjects: углеводы
сладкие газированные напитки
анкетирование
калорийность рациона

description: В статье представлены данные о частоте потребления углеводсодержащих сладких газированных напитков населением РФ и их вклад в общую калорийность рациона питания. Проведено анкетирование 11 850 лиц различного возраста (от 12 до 60 лет) и пола во всех 8 федеральных округах России. Изучали частоту потребления пищевых продуктов, а также параллельно собирали данные о фактическом питании методом 24-часового воспроизведения питания. Исследование показало достаточно низкую частоту потребления сладких газированных напитков и отсутствие существенных различий в частоте их потребления в различных федеральных округах России. С той или иной частотой потребляет сладкие газированные напитки от 55,5 до 67,3% населения, при этом 18,1–20,9% анкетированных лиц потребляют их не чаще 1–3 раз в месяц, а 1,3% обследованных (от 0,3% в Северо-Западном до 3,9% в Южном федеральном округе) – 2 раза в день или чаще. Анализ данных, полученных в результате проведенного анкетирования, показал, что вклад углеводного компонента, содержащегося в сладких газированных напитках, в различных округах России, даже при частом их потреблении (5–6 раз в неделю), не превышает 3,71% от общей калорийности рациона и не более 7,1% от калорийности углеводов в рационе питания.
Fractional calculus ties the microscopic and macroscopic scales of complex network dynamics
Creators: name: West, Bruce J.
name: Turalska, Malgorzata
name: Grigolini, Paolo
Publisher: name: arXiv
Year: 2014
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: A two-state master equation based decision making model has been shown to generate phase transitions, to be topologically complex and to manifest temporal complexity through an inverse power-law probability distribution function in the switching times between the two critical states of consensus. These properties are entailed by the fundamental assumption that the network elements in the decision making model imperfectly imitate one another. The process of subordination establishes that a single network element can be described by a fractional master equation whose analytic solution yields the observed inverse power-law probability distribution obtained by numerical integration of the two-state master equation to a high degree of accuracy.
An Information-Theoretic Approach to Transferability in Task Transfer Learning
Creators: name: Bao, Yajie
name: Li, Yang
name: Huang, Shao-Lun
name: Zhang, Lin
name: Zheng, Lizhong
name: Zamir, Amir
name: Guibas, Leonidas
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Task transfer learning is a popular technique in image processing applications that uses pre-trained models to reduce the supervision cost of related tasks. An important question is to determine task transferability, i.e. given a common input domain, estimating to what extent representations learned from a source task can help in learning a target task. Typically, transferability is either measured experimentally or inferred through task relatedness, which is often defined without a clear operational meaning. In this paper, we present a novel metric, H-score, an easily-computable evaluation function that estimates the performance of transferred representations from one task to another in classification problems using statistical and information theoretic principles. Experiments on real image data show that our metric is not only consistent with the empirical transferability measurement, but also useful to practitioners in applications such as source model selection and task transfer curriculum learning.
Additional file 1 of The impact of the temporary suspension of national cancer screening programmes due to the COVID-19 epidemic on the diagnosis of breast and colorectal cancer in the Netherlands
Creators: name: Dinmohamed, Avinash G.
name: Cellamare, Matteo
name: Visser, Otto
name: Munck, Linda De
name: Elferink, Marloes A. G.
name: Westenend, Pieter J.
name: Wesseling, Jelle
name: Broeders, Mireille J. M.
name: Kuipers, Ernst J.
name: Merkx, Matthias A. W.
name: Nagtegaal, Iris D.
name: Siesling, Sabine
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Methological details and additional results.
NASA KSC Railroad System Historical District
Creators: name: Historic American Engineering Record
Year: 2013
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: 8BR02932
valueUri: https://core.tdar.org/browse/site-name/116956/8br02932
subject: Road, Trail, and Related Structures or Features
valueUri: https://core.tdar.org/browse/site-type/294/road-trail-and-related-structures-or-features
subject: Railroad
valueUri: https://core.tdar.org/browse/site-type/298/railroad
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Historic Background Research
valueUri: https://core.tdar.org/browse/investigation-type/18/historic-background-research
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: Site form for BR02932.
Complete chloroplast genome sequence of Eranthis byunsanensis B.Y. Sun (Ranunculaceae), an endemic species in Korea
Creators: name: Park, Joon Moh
name: Oh, Ami
name: Koo, Jachoon
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology
subject: 60506 Virology

description: The Korean endemic Eranthis byunsanensis B.Y. Sun, 1993 (Ranunculaceae) is a rare plant distributed in the southwestern part of the Korean Peninsula. The complete chloroplast (cp) genome of E. byunsanensis was sequenced by next-generation sequencing (NGS) using an Illumina HiSeq X platform. The cp genome of E. byunsanensis is 160,324 bp in length with 37.9% GC content. It showed a typical quadripartite structure consisting of a pair of inverted repeats (IRs; 28,356 bp), a large single-copy region (LSC; 87,671 bp), and a small single-copy region (SSC; 15,941 bp). The cp genome comprises 130 genes including 85 protein-coding genes (PCGs), 37 tRNA genes, and eight rRNA genes. The molecular phylogenetic analysis indicates that E. byunsanensis is closely related to Eranthis stellata, both of which belong to the genus Eranthis.
Additional file 1 of Probing time-dependent afterslip and viscoelastic relaxation following the 2015 Mw7.8 Gorkha earthquake based on the 3-D finite-element model
Creators: name: Su, Lina
name: Fuqiang Shi
name: Weijun Gan
name: Xiaoning Su
name: Junyi Yan
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Additional file 1. Additional figures.
An Overdensity of Lyman Break Galaxies Around the Hot Dust-Obscured Galaxy WISE J224607.56$-$052634.9
Creators: name: Zewdie, Dejene
name: Assef, Roberto J.
name: Mazzucchelli, Chiara
name: Aravena, Manuel
name: Blain, Andrew W.
name: Díaz-Santos, Tanio
name: Eisenhardt, Peter R. M.
name: Jun, Hyunsung D.
name: Stern, Daniel
name: Tsai, Chao-Wei
name: Wu, "and" Jingwen W.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the identification of Lyman Break Galaxy (LBG) candidates around the most luminous Hot Dust-Obscured Galaxy (Hot DOG) known, WISE J224607.56$-$052634.9 (W2246$-$0526) at $z=4.601$, using deep \textit{r}-, \textit{i}-, and \textit{z}-band imaging from the Gemini Multi-Object Spectrograph South (GMOS-S). We use the surface density of LBGs to probe the Mpc-scale environment of W2246$-$0526 to characterize its richness and evolutionary state. We identify LBG candidates in the vicinity of W2246$-$0526 using the selection criteria developed by \cite{2004VOuchi} and \cite{2006Yoshida} in the Subaru Deep Field and in the Subaru XMM-Newton Deep Field, slightly modified to account for the difference between the filters used, and we find 37 and 55 LBG candidates, respectively. Matching to the $z$-band depths of those studies, this corresponds to $δ= 5.8^{+2.4}_{-1.9}$ times the surface density of LBGs expected in the field. Interestingly, the Hot DOG itself, as well as a confirmed neighbor, do not satisfy either LBG selection criteria, suggesting we may be missing a large number of companion galaxies. Our analysis shows that we are most likely only finding those with higher-than-average IGM optical depth or moderately high dust obscuration. The number density of LBG candidates is not concentrated around W2246$-$0526, suggesting either an early evolutionary stage for the proto-cluster or that the Hot DOG may not be the most massive galaxy, or that the Hot DOG may be affecting the IGM transparency in its vicinity. The overdensity around W2246$-$0526 is comparable to overdensities found around other Hot DOGs and is somewhat higher than typically found for radio galaxies and luminous quasars at a similar redshift.
description: 20 pages, 15 figures. The main results are in Figures 9 and 12. Accepted for publication in A&A
Optoelectromechanical transducer: reversible conversion between microwave and optical photons
Creators: name: Tian, Lin
Publisher: name: arXiv
Year: 2014
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Quantum states encoded in microwave photons or qubits can be effectively manipulated, whereas optical photons can be coherently transferred via optical fibre and waveguide. The reversible conversion of quantum states between microwave and optical photons will hence enable the distribution of quantum information over long distance and significantly improve the scalability of hybrid quantum systems. Owning to technological advances, mechanical resonators couple to quantum devices in distinctly different spectral range with tunable coupling, and can serve as a powerful interface to connect those devices. In this review, we summarize recent theory and experimental progress in the coherent conversion between microwave and optical fields via optoelectromechanical transducers. The challenges and perspectives in achieving single-photon-level quantum state conversion will also be discussed.
description: Review article, to appear in Annalen der Physik; 7 figures
Calibrating angular momentum transport in intermediate-mass stars from gravity-mode asteroseismology
Creators: name: Mombarg, Joey S. G.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The physical mechanisms driving the transport of angular momentum in stars are not fully understood, as current models cannot explain the observed stellar rotation profiles across all stages of evolution. By making use of pulsating F-type dwarfs, this work aims at (i) observationally calibrating the efficiency of angular momentum transport, assuming a constant uniform viscosity, and (ii) testing how well state-of-the-art rotating stellar models with angular momentum (AM) transport by rotationally-induced processes can explain observed rotation profiles. In both cases, the aim is to simultaneously reproduce the measured near-core rotation and core-to-surface rotation ratio. Asteroseismic modelling is applied to a sample of seven slowly rotating pulsators, to derive (core) masses and ages from their gravity-mode oscillations. This work focuses on the main sequence, using models that start with an initial uniform rotation frequency at the start of core-hydrogen burning that is a free parameter. Two treatments of AM transport are considered: (i) a constant uniform viscosity, and (ii) rotationally-induced processes. Next, the initial rotation frequency of each star is derived from the observed present-day near-core rotation frequency for both treatments. To explain the near-core rotation rate at the inferred age, initial rotation frequencies at the zero-age main sequence need to be below 10 percent of the initial critical break-up frequency. A diffusive approximation of angular momentum transport can in general explain the observed rotation profiles of the six slowly-rotating F-type dwarfs, for average values of the viscosity between 2x10^5 and 5x10^7 cm^2/s or when the viscosity is computed from rotationally-induced mechanisms. Yet, for three stars in the sample, the core-to-surface rotation fraction from rotationally-induced mechanisms is predicted to be higher than observed.
description: Accepted for publication in Astronomy & Astrophysics, 13 pages
Gas phase Elemental abundances in Molecular cloudS (GEMS) VIII. Unlocking the CS chemistry: the CH + S$\rightarrow$ CS + H and C$_2$ + S$\rightarrow$ CS + C reactions
Creators: name: Rocha, Carlos M. R.
name: Roncero, Octavio
name: Bulut, Niyazi
name: Zuchowski, Piotr
name: Navarro-Almaida, David
name: Fuente, Asuncion
name: Wakelam, Valentine
name: Loison, Jean-Christophe
name: Roueff, Evelyne
name: Goicoechea, Javier R.
name: Esplugues, Gisela
name: Beitia-Antero, Leire
name: Caselli, Paola
name: Lattanzi, Valerio
name: Pineda, Jaime
name: Gal, Romane Le
name: Rodriguez-Baras, Marina
name: Riviere-Marichalar, Pablo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We revise the rates of reactions CH + S -> CS + H and C_2 + S -> CS + C, important CS formation routes in dark and diffuse warm gas. We performed ab initio calculations to characterize the main features of all the electronic states correlating to the open shell reactants. For CH+S we have calculated the full potential energy surfaces for the lowest doublet states and the reaction rate constant with a quasi-classical method. For C_2+S, the reaction can only take place through the three lower triplet states, which all present deep insertion wells. A detailed study of the long-range interactions for these triplet states allowed to apply a statistic adiabatic method to determine the rate constants. This study of the CH + S reaction shows that its rate is nearly independent on the temperature in a range of 10-500 K with an almost constant value of 5.5 10^{-11} cm^3/s at temperatures above 100~K. This is a factor \sim 2-3 lower than the value obtained with the capture model. The rate of the reaction C_2 + S depends on the temperature taking values close to 2.0 10^{-10} cm^3/s at low temperatures and increasing to 5. 10^{-10} cm^3/s for temperatures higher than 200~K. Our modeling provides a rate higher than the one currently used by factor of \sim 2. These reactions were selected for involving open-shell species with many degenerate electronic states, and the results obtained in the present detailed calculations provide values which differ a factor of \sim 2-3 from the simpler classical capture method. We have updated the sulphur network with these new rates and compare our results in the prototypical case of TMC1 (CP). We find a reasonable agreement between model predictions and observations with a sulphur depletion factor of 20 relative to the sulphur cosmic abundance, but it is not possible to fit all sulphur-bearing molecules better than a factor of 10 at the same chemical time.
description: 13 pages, 10 figures
Tribal Letter: No Knowledge of any Archaeological Sites at Cape Canaveral Air Force Station
Creators: name: Terry, Steve
name: Dayhoff, Fred
Publisher: name: 45th Space Wing, USAF
Year: 2004
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Consultation
valueUri: https://core.tdar.org/browse/investigation-type/4/consultation

description: Correspondence from Miccosukee Tribe indicating the Tribe has no knowledge of any archaeological sites that would be on the base.
MOKA3D: An innovative approach to 3D gas kinematic modelling. I. Application to AGN ionized outflows
Creators: name: Marconcini, C.
name: Marconi, A.
name: Cresci, G.
name: Venturi, G.
name: Ulivi, L.
name: Mannucci, F.
name: Belfiore, F.
name: Tozzi, G.
name: Ginolfi, M.
name: Marasco, A.
name: Carniani, S.
name: Amiri, A.
name: Di Teodoro, E.
name: Scialpi, M.
name: Tomicic, N.
name: Mingozzi, M.
name: Brazzini, M.
name: Moreschini, B.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Studying the feedback process of Active Galactic Nuclei (AGN) requires characterising multiple kinematical components, such as rotating gas and stellar disks, outflows, inflows, and jets. To compare the observed properties with theoretical predictions of galaxy evolution and feedback models and to assess the mutual interaction and energy injection rate into the interstellar medium (ISM), one usually relies on simplified kinematic models. These models have several limitations, as they often do not take into account projection effects, beam smearing and the surface brightness distribution of the emitting medium. Here, we present MOKA3D, an innovative approach to model the 3D gas kinematics from integral field spectroscopy observations. In this first paper, we discuss its application to the case of AGN ionised outflows, whose observed clumpy emission and apparently irregular kinematics are only marginally accounted for by existing kinematical models. Unlike previous works, our model does not assume the surface brightness distribution of the gas, but exploits a novel procedure to derive it from the observations by reconstructing the 3D distribution of emitting clouds and providing accurate estimates of the spatially resolved outflow physical properties (e.g. mass rate, kinetic energy). As an example, we demonstrate the capabilities of our method by applying it to three nearby Seyfert-II galaxies observed with MUSE at the VLT and selected from the MAGNUM survey, showing that the complex kinematic features observed can be described by a conical outflow with a constant radial velocity field and a clumpy distribution of clouds.
description: 17 pages, 14 figures
The AstroSat observation of accreting millisecond X-ray pulsar SAX J1808.4-3658 during its 2019 outburst
Creators: name: Sharma, Rahul
name: Sanna, Andrea
name: Beri, Aru
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report on the analysis of the AstroSat dataset of the accreting millisecond X-ray pulsar SAX J1808.4-3658, obtained during its 2019 outburst. We found coherent pulsations at $\sim 401$ Hz and an orbital solution consistent with previous studies. The 3-20 keV pulse profile can be well fitted with three harmonically related sinusoidal components with background-corrected fractional amplitude of $\sim 3.5 \%$, $\sim 1.2 \%$ and $\sim 0.37 \%$ for fundamental, second and third harmonic, respectively. Our energy-resolved pulse profile evolution study indicate a strong energy dependence. We also observed a soft lag in fundamental and hard lag during its harmonic. The broadband spectrum of SAX J1808.4-3658 can be well described with a combination of thermal emission component with $kT \sim 1$ keV, a thermal Comptonization ($Γ\sim 1.67$) from the hot corona and broad emission lines due to Fe.
description: Accepted for publication in MNRAS
SHPO: Case Study for the Demolition of Facility 4120-Transformer Building (8BR2252), Launch Complex 1/2, Cape Canaveral Air Force Station
Creators: name: Penders, Thomas
Publisher: name: 45th Space Wing, USAF
Year: 2014
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: 8BR02248
valueUri: https://core.tdar.org/browse/site-name/116800/8br02248
subject: Launch Complex 1/2
valueUri: https://core.tdar.org/browse/site-name/117014/launch-complex-12
subject: 8BR02252
valueUri: https://core.tdar.org/browse/site-name/116874/8br02252
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Historic Background Research
valueUri: https://core.tdar.org/browse/investigation-type/18/historic-background-research
subject: Consultation
valueUri: https://core.tdar.org/browse/investigation-type/4/consultation
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: The 45th Space Wing (45 SW) of the United States Air Force (USAF) proposed to demolish Facility 4120-Transformer Building (8BR2252) at Launch Complex 1/2. The Florida SHPO concurred that the undertaking would be an adverse effect and requested a case study be prepared to demonstrate that all possible alternatives were addressed prior to the decision to demolish the properties. This case study has been prepared per the request of the Florida SHPO.
Scaling of magnetic reconnection in relativistic collisionless plasmas
Creators: name: Liu, Yi-Hsin
name: Guo, Fan
name: Daughton, William
name: Li, Hui
name: Hesse, Michael
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Using fully kinetic simulations, we study the scaling of the inflow speed of collisionless magnetic reconnection from the non-relativistic to ultra-relativistic limit. In the anti-parallel configuration, the inflow speed increases with the upstream magnetization parameter $σ$ and approaches the light speed when $σ> O(100)$, leading to an enhanced reconnection rate. In all regimes, the divergence of pressure tensor is the dominant term responsible for breaking the frozen-in condition at the x-line. The observed scaling agrees well with a simple model that accounts for the Lorentz contraction of the plasma passing through the diffusion region. The results demonstrate that the aspect ratio of the diffusion region remains $\sim 0.1$ in both the non-relativistic and relativistic limits.
description: 5 pages, 3 figures, submitted
Use of the directional atherectomy for the treatment of femoro-popliteal lesions in patients with critical lower limb ischemia
Creators: name: Bracale, Umberto Marcello
name: Vitale, Gaetano
name: Bajardi, Guido
name: Narese, Donatella
name: Dinoto, Ettore
name: Giribono, Anna Maria
name: Ferrara, Doriana
name: Del Guercio, Luca
name: Midiri, Massimo
name: Pecoraro, Felice
Publisher: name: Universita' degli Studi di Salerno
Year: 2016
Subjects: Turbohawk device
Critical limb ischemia
Atherectomy
Endovascular treatment

description: Femoro-popliteal PTA for the treatment of critical limb ischemia is frequently associated with unsatisfactory procedural success rates while directional atherectomy (DCA) has improved success rate since claudicant patients undergoing percutaneous treatment of femoro-popliteal obstructive disease. The aim of this prospective study is to evaluate the safety, efficacy and procedural success of DCA, at one year, in the percutaneous treatment of femoro-popliteal obstructive disease in patients with critical limb ischemia. Methods. From March 2012 to March 2013 18 consecutive patients with critical limb ischemia were treated with DCA (Turbohawk/Covidien-ev3 Endovascular Inc., North Plymouth, Minnesota, USA) for the treatment of femoro-popliteal obstructive disease. Patients were evaluated at 12 months. Results. Technical and procedural success was achieved in every patient. No in-hospital major adverse cardiovascular events occurred. Primary endpoint: freedom from any amputation was obtained in all patients. Secondary endpoints: clinical (Rutherford class improvement) and hemodynamic success (Ankle-brachial index improvement) was achieved in all patients. Conclusion. The use of DCA for the treatment of femoro-popliteal obstructive disease is a safe and effective therapeutic strategy for patients with critical limb ischemia. The data included in our study should be considered hypothesis-generating in order to design of a randomized trial comparison with conventional PTA.
Deformations of the Canonical Commutation Relations and Metric Structures
Creators: name: D'andrea, Francesco
name: Lizzi, Fedele
name: Martinetti, Pierre
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using Connes distance formula in noncommutative geometry, it is possible to retrieve the Euclidean distance from the canonical commutation relations of quantum mechanics. In this note, we study modifications of the distance induced by a deformation of the position-momentum commutation relations. We first consider the deformation coming from a cut-off in momentum space, then the one obtained by replacing the usual derivative on the real line with the h- and q-derivatives, respectively. In these various examples, some points turn out to be at infinite distance. We then show (on both the real line and the circle) how to approximate points by extended distributions that remain at finite distance. On the circle, this provides an explicit example of computation of the Wasserstein distance.
Historic Properties Investigations of a Proposed Security Fence for Fuel Storage Area #1, Cape Canaveral Air Force Station, Brevard County, Florida
Creators: name: Seckinger, Ernest W.
name: Robinson, Neil D.
Year: 1988
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Malabar II Cultures
valueUri: https://core.tdar.org/browse/culture-keyword/4943/malabar-ii-cultures
subject: 8BR00085
valueUri: https://core.tdar.org/browse/site-name/116100/8br00085
subject: Burns Mound
valueUri: https://core.tdar.org/browse/site-name/116169/burns-mound
subject: Burial Mound
valueUri: https://core.tdar.org/browse/site-type/303/burial-mound
subject: Fauna
valueUri: https://core.tdar.org/browse/material-type/4/fauna
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Methodology, Theory, or Synthesis
valueUri: https://core.tdar.org/browse/investigation-type/6/methodology-theory-or-synthesis
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing
subject: Systematic Survey
valueUri: https://core.tdar.org/browse/investigation-type/12/systematic-survey

description: Historic properties survey of the fence alignment and a Phase II cultural resource survey of that portion of archeological site 8Br85 said to lie within the project area of the new fence.
Origins of the U.S. genre-fiction system, 1890–1956
Creators: name: Goldstone, Andrew
Publisher: name: Rutgers University
Year: 2023
Subjects: Sociology of Culture
American Literature
Publishing

description: Though genre fiction is now ubiquitous, and though both book history and literary studies have devoted considerable attention to individual genres like science fiction and romance novels, the history of the system of popular fiction categories has been little studied. This essay traces the origins of the genre-fiction system in United States magazine and book publishing, bringing sociological and book-historical analysis to bear on changing practices of categorization in publishing, advertising, librarianship, and reader response from the 1890s through the 1950s. Genre categories were only intermittently in use through the 1910s; they were first institutionalized in pulp magazines in the 1920s and 1930s. The genre-fiction system was transmitted to book publishing only in the course of the so-called "paperback revolution" of the 1940s and 1950s, which made room for fiction-book production by categories while relegating it to a permanently low-status position. This transmission across publishing formats was far from deliberate; instead, the essay argues, the system of genre fiction arose and endured as a stable compromise articulating an expanded fiction-reading public to an expansive print culture industry, making new readers and new fiction—and new kinds of fiction—regularly available to each other in an enduringly hierarchized field.
Stochastic star formation in early galaxies: JWST implications
Creators: name: Pallottini, A.
name: Ferrara, A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The star formation rate (SFR) in high redshift galaxies is expected to be time-variable due to competing physical processes. Such stochastic variability might boost the luminosity of galaxies, possibly explaining the over-abundance seen at $z\gtrsim 10$ by JWST. We aim at quantifying the amplitude and timescales of such variability, and identifying the key driving physical processes. We select 245 $z=7.7$ galaxies with stellar mass $5\times 10^{6}\lesssim M_\star/{\rm M}_\odot\lesssim 5\times 10^{10}$ from SERRA, a suite of high-resolution, radiation-hydrodynamic cosmological simulations. After fitting the average SFR trend, $\langle {\rm SFR} \rangle$, we quantify the time-dependent variation, $δ(t) \equiv \log [\rm SFR/\langle {\rm SFR} \rangle]$ for each system, and perform a periodogram analysis to search for periodicity modulations. We find that $δ(t)$ is distributed as a zero-mean Gaussian, with standard deviation $σ_δ\simeq 0.24$ (corresponding to a UV magnitude s.d. $σ_{\rm UV} \simeq 0.61$) that is independent of $M_\star$. However, the modulation timescale increases with stellar mass: $t_δ\sim (9, 50, 100)\, \rm Myr$ for $M_\star \sim (0.1, 1, 5)\times 10^9\, {\rm M}_\odot$, respectively. These timescales are imprinted on the SFR by different processes: (i) photoevaporation, (ii) supernova explosions, and (iii) cosmological accretion/merging dominating in low, intermediate, and high mass systems, respectively. The predicted SFR variations cannot account for the required $z\gtrsim 10$ UV luminosity function boost. Other processes, such as radiation-driven outflows clearing the dust, must then be invoked to explain the enhanced luminosity of super-early systems.
description: 5 pages, 4 figures, accepted by A&A
Visual Transformers for Primates Classification and Covid Detection
Creators: name: Illium, Steffen
name: Müller, Robert
name: Sedlmeier, Andreas
name: Popien, Claudia-Linnhoff
Publisher: name: arXiv
Year: 2022
Subjects: subject: Sound (cs.SD)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Audio and Speech Processing (eess.AS)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: We apply the vision transformer, a deep machine learning model build around the attention mechanism, on mel-spectrogram representations of raw audio recordings. When adding mel-based data augmentation techniques and sample-weighting, we achieve comparable performance on both (PRS and CCS challenge) tasks of ComParE21, outperforming most single model baselines. We further introduce overlapping vertical patching and evaluate the influence of parameter configurations. Index Terms: audio classification, attention, mel-spectrogram, unbalanced data-sets, computational paralinguistics
Calibration of the ICARUS cryogenic photo-detection system at FNAL
Creators: name: Bonesini, M.
name: Benocci, R.
name: Bertoni, R.
name: Chatterjee, A.
name: Diwan, M.
name: Menegolli, A.
name: Raselli, G.
name: Rossella, M.
name: Scarpelli, A.
name: Suarez, N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The calibration of the ICARUS photo-detection system is based on a low power laser diode at 405 nm. Laser pulses arrive to one optical switch and then are sent to 36 UHV flanges, by 20 meters long optical patches. Light is then delivered to the ten PMTs connected to a single flange, by 7m long injection optical patches. Extensive tests of the used components and care in the design of the optical system have guaranteed to each PMT a sizeable calibration signal with minimal distortion, with respect to the original one. Gain equalization of PMTs has reached a 1 per cent resolution. In this procedure data from background photons were also used. The distribution of the PMTs signal arrival time has a distribution with a resolution less than 1 ns, thus allowing a good determination of the absolute event timing. The status of the laser calibration system with its possible upgrades will be reported.
Exploring the chemodynamics of metal-poor stellar populations
Creators: name: da Silva, André Rodrigo
name: Smiljanic, Rodolfo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Metal-poor stars are key for studying the formation and evolution of the Galaxy. Evidence of the early mergers that built up the Galaxy remains in the distributions of abundances, kinematics, and orbital parameters of its stars. Several substructures resulting from these mergers have been tentatively identified in the literature. We conduct a global analysis of the chemodynamic properties of metal-poor stars. Our aim is to identify signs of accreted and in situ stars in different regions of the parameter space and to investigate their differences and similarities. We selected a sample of about 6600 metal-poor stars with [Fe/H] $\leq$ -0.8 from DR3 of the GALAH survey. We used unsupervised machine learning to separate stars in a parameter space made of two normalised orbital actions, plus [Fe/H] and [Mg/Fe], without additional a priori cuts on stellar properties. We divided the halo stars in four main groups. All groups exhibit a significant fraction of in situ contamination (ISC). Accreted stars of these groups have very similar chemical properties, except for those of the group of stars with very retrograde orbits. This points to at most two main sources of accreted stars in the current sample, the major one related to Gaia-Enceladus (GE) and the other possibly related to Thamnos and/or Sequoia. Stars of GE are r-process enriched at low metallicities, but a contribution of the s-process appears with increasing metallicity. A flat trend of [Eu/Mg] as a function of [Fe/H] suggests that only core collapse supernovae contributed to r-process elements in GE. To better characterise accreted stars in the low metallicity regime, high precision abundances and guidance from chemical evolution models are needed. It is possible that ISC in samples of accreted stars has been underestimated. This can have important consequences for attempts to estimate the properties of the original systems.
description: 22 pages, 22 figures, Accepted for publication in A&A
Historic American Engineering Record Documentation of Launch Complex 9/10 Cape Canaveral Air Force Station, Brevard County, Florida
Creators: name: Enscore, Susan I.
name: Hinder, Kimberly
Publisher: name: Historic American Engineering Record, National Park Service
Year: 2016
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Cold War
valueUri: https://core.tdar.org/browse/temporal-keyword/7288/cold-war
subject: Launch Complex 9 & 10
valueUri: https://core.tdar.org/browse/site-name/116393/launch-complex-9-10
subject: Jason
valueUri: https://core.tdar.org/browse/other-keyword/164464/jason
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Alpha Draco
valueUri: https://core.tdar.org/browse/other-keyword/164465/alpha-draco
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Historic Background Research
valueUri: https://core.tdar.org/browse/investigation-type/18/historic-background-research
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: HAER documentation of Launch Complex 9/10 located on Cape Canaveral Air Force Station, Florida. This record contains written, graphic, and photographic material as required for mitigation when a significant historic resource is altered or demolished. Constructed 1953-1957, Launch Complex 9/10 at Cape Canaveral Air Force Station was designed to support the Air Force's Navaho winged intercontinental missile. Although the program was cancelled soon after completion of the complex, test flights continued until November 1958. Launch Pad 10 served as the test site for the Navaho, the Jason research rocket, and the Alpha Draco missile.
Historic Resources Survey: Payload Spintest Facility, Cape Canaveral Air Force Station, Brevard County, Florida
Creators: name: Seckinger, Ernie
name: Neilsen, Jerry
Year: 1991
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Payload Spintest Facility
valueUri: https://core.tdar.org/browse/site-name/116124/payload-spintest-facility
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking
subject: Systematic Survey
valueUri: https://core.tdar.org/browse/investigation-type/12/systematic-survey

description: This report summarizes the results of a Phase I historic resources survey in support of the Payload Spintest Support Facility (PSSF). The survey covered 6.6 acres. The results of this project are summarized in two separate volumes, an architectural and engineering survey and an archaeological survey. This project did not identify any known sites or space related engineering elements within the project area.
Test Case Purification for Improving Fault Localization
Creators: name: Xuan, Jifeng
name: Monperrus, Martin
Publisher: name: arXiv
Year: 2014
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Finding and fixing bugs are time-consuming activities in software development. Spectrum-based fault localization aims to identify the faulty position in source code based on the execution trace of test cases. Failing test cases and their assertions form test oracles for the failing behavior of the system under analysis. In this paper, we propose a novel concept of spectrum driven test case purification for improving fault localization. The goal of test case purification is to separate existing test cases into small fractions (called purified test cases) and to enhance the test oracles to further localize faults. Combining with an original fault localization technique (e.g., Tarantula), test case purification results in better ranking the program statements. Our experiments on 1800 faults in six open-source Java programs show that test case purification can effectively improve existing fault localization techniques.
SHPO: Development of the Cape Canaveral Lighthouse (8BR212) and New Lighthouse Site (8BR1660), Cape Canaveral Air Force Station (CCAFS), Brevard County Florida
Creators: name: Blaylock, Michael A.
Year: 2014
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: 8BR00212
valueUri: https://core.tdar.org/browse/site-name/116095/8br00212
subject: 8BR01660
valueUri: https://core.tdar.org/browse/site-name/116348/8br01660
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Consultation
valueUri: https://core.tdar.org/browse/investigation-type/4/consultation
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: SHPO Correspondence regarding the final site plan for the development of the Cape Canaveral Lighthouse (8BR212) and the New Lighthouse (8BR1160).