cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Cape Canaveral Air Force Station General Plan
Creators: name: 45 SW
Year: 2011
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

description: The Cape Canaveral Air Force Station (CCAFS) General Plan (Plan) presents a condensed picture of the present and future capability of the installation to support the 45th Space Wing (45 SW) mission and to ensure United States (U.S.) access to space. The Plan is a summary document that includes a systematic framework of comprehensive planning information with regard to short term and long term installation development. It provides information at an appropriate level of detail for command and other decision makers to understand the character and structure of the installation and its development potential. The Plan incorporates currently identified projects, anticipates future program requirements, and ensures compliance with applicable Federal, state and local laws, regulations and policies. The Plan summarizes an assessment of the installation’s infrastructure, natural resources and land uses for the purpose of gauging development potential. The Plan is a roadmap that guides the 45 SW to efficiently utilize land, allocate infrastructure resources and provide flexibility to meet current and evolving mission requirements.
van_den_Heuvel_tables_figures_ESM from Artificial selection for reversal learning reveals limited repeatability and no heritability of cognitive flexibility in great tits (Parus major)
Creators: name: van den Heuvel, Krista
name: Quinn, John L.
name: Kotrschal, Alexander
name: van Oers, Kees
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences
classificationCode: 170299
subject: Cognitive Science not elsewhere classified
classificationCode: 60801
subject: Animal Behaviour

description: Cognitive flexibility controls how animals respond to changing environmental conditions. Individuals within species vary considerably in cognitive flexibility but the micro-evolutionary potential in animal populations remains enigmatic. One prerequisite for cognitive flexibility to be able to evolve is consistent and heritable among-individual variation. Here we determine the repeatability and heritability of cognitive flexibility among great tits (Parus major) by performing an artificial selection experiment on reversal learning performance using a spatial learning paradigm over three generations. We found low, yet significant, repeatability (R = 0.15) of reversal learning performance. Our artificial selection experiment showed no evidence for narrow-sense heritability of associative or reversal learning, while we confirmed the heritability of exploratory behaviour. We observed a phenotypic, but no genetic, correlation between associative and reversal learning, showing the importance of prior information on reversal learning. We found no correlation between cognitive and personality traits. Our findings emphasize that cognitive flexibility is a multi-faceted trait that is affected by memory and prior experience, making it challenging to retrieve reliable values of temporal consistency and assess the contribution of additive genetic variation. Future studies need to identify what cognitive components underly variation in reversal learning and study their between-individual and additive genetic components.
Launch Complex 37 Maps and Illustrations
Creators: name: Maurice H. Connell & Associates
name: Reynolds, Smith & Mills
Year: 1961
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 37
valueUri: https://core.tdar.org/browse/site-name/116301/launch-complex-37
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: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: Maps and Illustrations of Launch Complex 37.
Cape Canaveral Air Force Station 1950 Maps
Creators: name: Parsons Aerojet Company
Year: 1950
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: Maps
valueUri: https://core.tdar.org/browse/other-keyword/438/maps
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation

description: Maps of Cape Canaveral AFS from the 1950s.
MUSE-ALMA Halos XI: Gas flows in the circumgalactic medium
Creators: name: Weng, Simon
name: Péroux, Céline
name: Karki, Arjun
name: Augustin, Ramona
name: Kulkarni, Varsha P.
name: Hamanowicz, Aleksandra
name: Zwaan, Martin
name: Sadler, Elaine M.
name: Nelson, Dylan
name: Hayes, Matthew J.
name: Kacprzak, Glenn G.
name: Fox, Andrew J.
name: Bollo, Victoria
name: Casavecchia, Benedetta
name: Szakacs, Roland
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The flow of gas into and out of galaxies leaves traces in the circumgalactic medium which can then be studied using absorption lines towards background quasars. We analyse 27 log(N_HI) > 18.0 HI absorbers at z = 0.2 to 1.4 from the MUSE-ALMA Halos survey with at least one galaxy counterpart within a line of sight velocity of +/-500 km s^{-1}. We perform 3D kinematic forward modelling of these associated galaxies to examine the flow of dense, neutral gas in the circumgalactic medium. From the VLT/MUSE, HST broadband imaging and VLT/UVES and Keck/HIRES high-resolution UV quasar spectroscopy observations, we compare the impact parameters, star-formation rates and stellar masses of the associated galaxies with the absorber properties. We find marginal evidence for a bimodal distribution in azimuthal angles for strong HI absorbers, similar to previous studies of the MgII and OVI absorption lines. There is no clear metallicity dependence on azimuthal angle and we suggest a larger sample of absorbers are required to fully test the relationship predicted by cosmological hydrodynamical simulations. A case-by-case study of the absorbers reveals that ten per cent of absorbers are consistent with gas accretion, up to 30 per cent trace outflows while the remainder trace gas in the galaxy disk, the intragroup medium and low-mass galaxies below the MUSE detection limit. Our results highlight that the baryon cycle directly affects the dense neutral gas required for star-formation and plays a critical role in galaxy evolution.
description: 13 pages, 6 figures, 12 pages of appendix. Accepted for publication in MNRAS
Journal of the Lighthouse Board
Creators: name: The Lighthouse Board
Year: 1893
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: Lighthouse
valueUri: https://core.tdar.org/browse/site-name/1150/lighthouse
subject: 8BR00212
valueUri: https://core.tdar.org/browse/site-name/116095/8br00212
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: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: Handwritten journal of the Lighthouse board from 1983.
Filling in the Gaps: Can Gravitationally Unstable Discs Form the Seeds of Gas Giant Planets?
Creators: name: Baehr, Hans
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Circumstellar discs likely have a short window when they are self-gravitating and prone to the effects of disc instability, but during this time the seeds of planet formation can be sown. It has long been argued that disc fragmentation can form large gas giant planets at wide orbital separations, but its place in the planet formation paradigm is hindered by a tendency to form especially large gas giants or brown dwarfs. We instead suggest that planet formation can occur early in massive discs, through the gravitational collapse of dust which can form the seeds of giant planets. This is different from the usual picture of self-gravitating discs, in which planet formation is considered through the gravitational collapse of the gas disc into a gas giant precursor. It is familiar in the sense that the core is formed first, and gas is accreted thereafter, as is the case in the core accretion scenario. However, by forming a $\sim 1 M_{\oplus}$ seed from the gravitational collapse of dust within a self-gravitating disc there exists the potential to overcome traditional growth barriers and form a planet within a few times $10^5$ years. The accretion of pebbles is most efficient with centimetre-sized dust, but the accretion of millimetre sizes can also result in formation within a Myr. Thus, if dust can grow to these sizes, planetary seeds formed within very young, massive discs could drastically reduce the timescale of planet formation and potentially explain the observed ring and gap structures in young discs.
description: MNRAS accepted. 15 pages, 12 figures
Survey Data from 1950 to 1969, Cape Canaveral
Creators: name: U.S. Army Corps Of Engineers
Year: 1969
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: Maps
valueUri: https://core.tdar.org/browse/other-keyword/438/maps
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
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: Survey Data from 1950 to 1969, Cape Canaveral.
Launch Complex 40 and 41, Illustrations and Photos
Creators: name: Pan American World Airways Inc.
Year: 1965
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 40
valueUri: https://core.tdar.org/browse/site-name/116416/launch-complex-40
subject: Launch Complex 41
valueUri: https://core.tdar.org/browse/site-name/117500/launch-complex-41
subject: Titan III
valueUri: https://core.tdar.org/browse/other-keyword/164622/titan-iii
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Remote Sensing
valueUri: https://core.tdar.org/browse/investigation-type/22/remote-sensing

description: Illustrations of Launch Complex 41.
Cape Kennedy Air Force Station Master Plan
Creators: name: Department Of The Air Force
Year: 1965
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: BIGS
valueUri: https://core.tdar.org/browse/other-keyword/164553/bigs
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Remote Sensing
valueUri: https://core.tdar.org/browse/investigation-type/22/remote-sensing
subject: Geophysical Survey
valueUri: https://core.tdar.org/browse/investigation-type/23/geophysical-survey
subject: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: Master plan for Cape Kennedy Air Force Station. This plan modifies the 1964 plan to reflect changes in scope and magnitude of guided missile, satellite, and space vehicle programs operated from the Eastern Test Range.
Aerial Images, Cape Canaveral (1979-1983 & 1993)
Creators: name: United States Geological Survey
Year: 1993
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: Aerial Imagery
valueUri: https://core.tdar.org/browse/other-keyword/110182/aerial-imagery
subject: Remote Sensing
valueUri: https://core.tdar.org/browse/investigation-type/22/remote-sensing

description: Aerial Images of Cape Canaveral (1979-1983 & 1993)
Continuous excitations of the triangular-lattice quantum spin liquid YbMgGaO4
Creators: name: Paddison, J. A. M.
name: Daum, M.
name: Dun, Z. L.
name: Ehlers, G.
name: Liu, Y.
name: Stone, M. B.
name: Zhou, H. D.
name: Mourigal, M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A quantum spin liquid (QSL) is an exotic state of matter in which electrons' spins are quantum entangled over long distances, but do not show symmetry-breaking magnetic order in the zero-temperature limit. The observation of QSL states is a central aim of experimental physics, because they host collective excitations that transcend our knowledge of quantum matter; however, examples in real materials are scarce. Here, we report neutron-scattering measurements on YbMgGaO4, a QSL candidate in which Yb3+ ions with effective spin-1/2 occupy a triangular lattice. Our measurements reveal a continuum of magnetic excitations - the essential experimental hallmark of a QSL - at very low temperature (0.06 K). The origin of this peculiar excitation spectrum is a crucial question, because isotropic nearest-neighbor interactions do not yield a QSL ground state on the triangular lattice. Using measurements of the magnetic excitations close to the field-polarized state, we identify antiferromagnetic next-nearest-neighbor interactions in the presence of planar anisotropy as key ingredients for QSL formation in YbMgGaO4.
description: 21 pages, 8 figures, includes Supplementary Information
Parameter estimates in binary black hole collisions using neural networks
Creators: name: Carrillo, M.
name: Gracia-Linares, M.
name: González, J. A.
name: Guzmán, F. S.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present an algorithm based on artificial neural networks (ANNs), that estimates the mass ratio in a binary black hole collision out of given Gravitational Wave (GW) strains. In this analysis, the ANN is trained with a sample of GW signals generated with numerical simulations. The effectiveness of the algorithm is evaluated with GWs generated also with simulations for given mass ratios unknown to the ANN. We measure the accuracy of the algorithm in the interpolation and extrapolation regimes. We present the results for noise free signals and signals contaminated with Gaussian noise, in order to foresee the dependence of the method accuracy in terms of the signal to noise ratio.
description: 7 pages, 9 eps figures
Black Hole Feeding and Feedback in a Compact Galaxy
Creators: name: Di, Yihuan
name: Li, Yuan
name: Yuan, Feng
name: Shi, Fangzheng
name: Caradonna, Mirielle
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We perform high-resolution hydrodynamical simulations using the framework of {\it MACER} to investigate supermassive black hole (SMBH) feeding and feedback in a massive compact galaxy, which has a small effective radius but a large stellar mass, with a simulation duration of 10 Gyr. We compare the results with a reference galaxy with a similar stellar mass but a less concentrated stellar density distribution, as typically found in local elliptical galaxies. We find that about 10% of the time, the compact galaxy develops multi-phase gas within a few kpc, but the accretion flow through the inner boundary below the Bondi radius is always a single phase. The inflow rate in the compact galaxy is several times larger than in the reference galaxy, mainly due to the higher gas density caused by the more compact stellar distribution. Such a higher inflow rate results in stronger SMBH feeding and feedback and a larger fountain-like inflow-outflow structure. Compared to the reference galaxy, the star formation rate in the compact galaxy is roughly two orders of magnitude higher but is still low enough to be considered quiescent. Over the whole evolution period, the black hole mass grows by $\sim$50% in the compact galaxy, much larger than the value of $\sim$ 3% in the reference galaxy.
description: 7 pages, 6 figures
Properties and Asteroseismological analysis of a new ZZ ceti discovered by TMTS
Creators: name: Guo, Jincheng
name: Chen, Yanhui
name: Wang, Xiaofeng
name: Lin, Jie
name: Xi, Gaobo
name: Mo, Jun
name: Filippenko, Alexei V.
name: Brink, Thomas
name: Ma, Xiao-Yu
name: Zong, Weikai
name: Yang, Yong
name: Zhao, Jingkun
name: Zeng, Xiangyun
name: Chen, Zhihao
name: Esamdin, Ali
name: Guo, Fangzhou
name: Iskandar, Abdusamatjan
name: Jiang, Xiaojun
name: Li, Wenxiong
name: Liu, Cheng
name: Shi, Jianrong
name: Song, Xuan
name: Wang, Letian
name: Xiang, Danfeng
name: Yan, Shengyu
name: Zhang, Jicheng
name: Yang, Yonghui
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Tsinghua university-Ma Huateng Telescope for Survey (TMTS) aims to discover rapidly evolving transients by monitoring the northern sky. The TMTS catalog is cross-matched with the white dwarf (WD) catalog of Gaia EDR3, and light curves of more than a thousand WD candidates are obtained so far. Among them, the WD TMTS J23450729+5813146 (hereafter J2345) is one interesting common source. Based on the light curves from the TMTS and follow-up photometric observations, periods of 967.113 s, 973.734 s, 881.525 s, 843.458 s, 806.916 s and 678.273 s are identified. In addition, the TESS observations suggest a 3.39 h period but this can be attributed to the rotation of a comoving M dwarf located within 3". The spectroscopic observation indicates that this WD is DA type with Teff = 11778+/-617K,log g = 8.38+/-0.31,mass=0.84+/-0.20Msun and age=0.704+/-0.377 Gyrs. Asteroseismological analysis reveals a global best-fit solution of Teff =12110+/-10K and mass=0.760+/-0.005Msun,consistent with the spectral fitting results, and Oxygen and Carbon abundances in the core center are 0.73 and 0.27, respectively. The distance derived from the intrinsic luminosity given by asteroseismology is 93 parsec, which is in agreement with the distance of 98 parsec from Gaia DR3. Additionally, kinematic study shows that this WD is likely a thick disk star. The mass of its zero-age main-sequence mass is estimated to be 3.08 Msun and has a main-sequence plus cooling age of roughly 900 Myrs.
description: 10 pages, 10 figures, accepted for publication in MNRAS
Solitons of a vector model on the honeycomb lattice
Creators: name: Vekslerchik, V. E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 35Q51, 35C08, 11C20

description: We study a simple nonlinear vector model defined on the honeycomb lattice. We propose a bilinearization scheme for the field equations and demonstrate that the resulting system is closely related to the well-studied integrable models, such as the Hirota bilinear difference equation and the Ablowitz-Ladik system. This result is used to derive the N-soliton solutions.
Launch Complex 37 Service Structure, Base Building, Machinery Building Maps
Creators: name: Maurice H. Connell & Associates
name: Reynolds, Smith & Mills
Year: 1961
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 37
valueUri: https://core.tdar.org/browse/site-name/116301/launch-complex-37
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: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: Maps and Illustrations of Launch Complex 37.
Launch Complex 20 Illustrations
Creators: name: Pan American World Airways Inc.
Year: 1964
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 20
valueUri: https://core.tdar.org/browse/site-name/116448/launch-complex-20
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: Remote Sensing
valueUri: https://core.tdar.org/browse/investigation-type/22/remote-sensing

description: Launch Complex 20 illustrations and photographs.
Titan III, Program 624A, Technical Launch Facilities
Creators: name: Rader And Associates
Year: 1968
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 41
valueUri: https://core.tdar.org/browse/site-name/117500/launch-complex-41
subject: Titan III
valueUri: https://core.tdar.org/browse/other-keyword/164622/titan-iii
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: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: Illustrations of Launch Complex 41.
Chemodynamical Properties and Ages of Metal-Poor Stars in S-PLUS
Creators: name: Almeida-Fernandes, Felipe
name: Placco, Vinicius
name: Rocha-Pinto, Helio
name: Fernandes, Marcelo Borges
name: Limberg, Guilherme
name: Silva, Leandro Beraldo e
name: Amarante, João A. S.
name: Perottoni, Hélio
name: Overzier, Roderik
name: Schoenell, William
name: Ribeiro, Tiago
name: Kanaan, Antonio
name: de Oliveira, Claudia Mendes
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Metal-poor stars are key to our understanding of the early stages of chemical evolution in the Universe. New multi-filter surveys, such as the Southern Photometric Local Universe Survey (S-PLUS), are greatly advancing our ability to select low-metallicity stars. In this work, we analyse the chemodynamical properties and ages of 522 metal-poor candidates selected from the S-PLUS data release 3. About 92% of these stars were confirmed to be metal-poor ([Fe/H] $\leq -1$) based on previous medium-resolution spectroscopy. We calculated the dynamical properties of a subsample containing 241 stars, using the astrometry from Gaia Data Release 3. Stellar ages are estimated by a Bayesian isochronal method formalized in this work. We analyse the metallicity distribution of these metal-poor candidates separated into different subgroups of total velocity, dynamical properties, and ages. Our results are used to propose further restrictions to optimize the selection of metal-poor candidates in S-PLUS. The proposed astrometric selection ($\mathrm{parallax}>0.85$ mas) is the one that returns the highest fraction of extremely metal-poor stars (16.3% have [Fe/H] $\leq -3$); the combined selection provides the highest fraction of very metal-poor stars (91.0% have [Fe/H] $\leq -2$), whereas the dynamical selection (eccentricity > 0.35 and diskness < 0.75) is better for targetting metal-poor (99.5% have [Fe/H] $\leq -1$). Using only S-PLUS photometric selections, it is possible to achieve selection fractions of 15.6%, 88.5% and 98.3% for metallicities below $-$3, $-$2 and $-$1, respectively. We also show that it is possible to use S-PLUS to target metal-poor stars in halo substructures such as Gaia-Sausage/Enceladus, Sequoia, Thamnos and the Helmi stream.
description: 18 pages, 13 figures. To be published in MNRAS main journal (accepted 15-may-2023)
Plus Charge Prevalence in Cosmic Rays: Room for Dark Matter in the Positron Spectrum
Creators: name: Malkov, M. A.
name: Diamond, P. H.
name: Sagdeev, R. Z.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The unexpected energy spectrum of the positron/electron ratio is interpreted astrophysically, with a possible exception of the 100-300 GeV range. The data indicate that this ratio, after a decline between $0.5-8$ GeV, rises steadily with a trend towards saturation at 200-400GeV. These observations (except for the trend) appear to be in conflict with the diffusive shock acceleration (DSA) mechanism, operating in a \emph{single} supernova remnant (SNR) shock. We argue that $e^{+}/e^{-}$ ratio can still be explained by the DSA if positrons are accelerated in a \emph{subset} of SNR shocks which: (i) propagate in clumpy gas media, and (ii) are modified by accelerated CR \emph{protons}. The protons penetrate into the dense gas clumps upstream to produce positrons and, \emph{charge the clumps positively}. The induced electric field expels positrons into the upstream plasma where they are shock-accelerated. Since the shock is modified, these positrons develop a harder spectrum than that of the CR electrons accelerated in other SNRs. Mixing these populations explains the increase in the $e^{+}/e^{-}$ ratio at $E>8$ GeV. It decreases at $E<8$ GeV because of a subshock weakening which also results from the shock modification. Contrary to the expelled positrons, most of the antiprotons, electrons, and heavier nuclei, are left unaccelerated inside the clumps. Scenarios for the 100-300 GeV AMS-02 fraction exceeding the model prediction, including, but not limited to, possible dark matter contribution, are also discussed.
description: 36 pages, 6 figures
Lone Cistern Site (8BR01935)
Creators: name: Penders, Thomas
name: Sutherland, Robin
name: Gaske, Frederick P.
Publisher: name: Florida Division of Historical Resources
Year: 2007
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: 8BR01935
valueUri: https://core.tdar.org/browse/site-name/116237/8br01935
subject: Lone Cistern Site
valueUri: https://core.tdar.org/browse/site-name/117024/lone-cistern-site
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
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
subject: Reconnaissance / Survey
valueUri: https://core.tdar.org/browse/investigation-type/7/reconnaissance-survey
subject: Site Evaluation / Testing
valueUri: https://core.tdar.org/browse/investigation-type/10/site-evaluation-testing

description: Documents, letters and photos associated with the Lone Cistern Site, 8BR01935.
Evidence of AGB pollution in Galactic globular clusters from the Mg-Al anticorrelations observed by the APOGEE survey
Creators: name: Ventura, P.
name: García--Hernández, D. A.
name: Dell'Agli, F.
name: D'Antona, F.
name: Meszaros, Sz.
name: Lucatello, S.
name: Di Criscienzo, M.
name: Shetrone, M.
name: Tailo, M.
name: Tang, Baitian
name: Zamora, O.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the formation of multiple populations in globular clusters (GC), under the hypothesis that stars in the second generation formed from the winds of intermediate-mass stars, ejected during the asymptotic giant branch (AGB) phase, possibly diluted with pristine gas, sharing the same chemical composition of first-generation stars. To this aim, we use the recent APOGEE data, which provide the surface chemistry of a large sample of giant stars, belonging to clusters that span a wide metallicity range. The APOGEE data set is particularly suitable to discriminate among the various pollution scenarios proposed so far, as it provides the surface abundances of Mg and Al, the two elements involved in a nuclear channel extremely sensitive to the temperature, hence to the metallicity of the polluters. The present analysis shows a remarkable agreement between the observations and the theoretical yields from massive AGB stars. In particular, the observed extension of the depletion of Mg and O and the increase in Al is well reproduced by the models and the trend with the metallicity is also fully accounted for. This study further supports the idea that AGB stars were the key players in the pollution of the intra-cluster medium, from which additional generations of stars formed in GC.
description: Accepted on ApJ letters
Testing Multiband (G, GBP, GRP, B, V and TESS) Standard Bolometric Corrections by Recovering Luminosity and Radii of 341 Host Stars
Creators: name: Eker, Zeki
name: Bakis, Volkan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Main-sequence bolometric corrections (BC) and a standard BC-Teff relation are produced for TESS wavelengths using published physical parameters and light ratios from SED models of 209 detached double-lined eclipsing binaries. This and previous five-band (Johnson B, V, Gaia G, GBP, GRP) standard BC-Teff relations are tested by recovering luminosity (L) of the most accurate 341 single host stars (281 MS, 40 subgiants, 19 giants and one PMS). The recovered L of photometry is compared to L from published R and Teff. A very high correlation ($R^2$ = 0.9983) is achieved for this mixed sample. Error histograms of recovered and calculated L show peaks at 2 and 4 per cent respectively. The recovered L and the published Teff} were then used in $L = 4 πR^2 σTeff^4$ to predict the standard R of the host stars. Comparison between the predicted and published R of all luminosity classes are found successful with a negligible offset associated with the giants and subgiants. The peak of the predicted R errors is found at 2 per cent, which is equivalent to the peak of the published R errors. Thus, a main-sequence BC-Teff relation could be used in predicting both L and R of a single star at any luminosity class, but this does not mean BC-Teff relations of all luminosity classes are the same because luminosity information could be more constrained by star's apparent magnitude $ξ$ than its BC since $m_{Bol} = ξ+ BC_ξ$.
description: 11 pages, 9 figures, a total of 6 tables, 5 online only tables
Market-Based Flexibility Services for Congestion Management
Creators: name: Brummund, David
name: Milzer, Gesa
name: Kratsch, Paul
Publisher: name: Zenodo
Year: 2023

description: According to the European Clean Energy Package (2019)
 Distribution System Operators (DSOs) shall effectively use
 flexibility services from local and regional assets to safely
 host more renewable energy sources in the electricity grid.
 Electricity prosumers become crucial players due to their
 potential to provide flexibility by adapting their
 production and consumption behaviour. Yet, integrating
 new types of assets into the distribution grid to use
 flexibility creates complexity and hardly predictable
 power flows in the distribution networks. The European
 H2020 demonstration project EUniversal aims to
 overcome the existing limitations in the use of flexibility.
 For that purpose, smart grid tools for grid state
 assessment and active system management are developed.
 A demonstration pilot is set up to test the flexibility value
 chain from congestion detection to market-based flexibility
 procurement via a local flexibility market. The pilot is
 conducted in the LV grids of the German DSO MITNETZ
 STROM, examining the use of flexible resources in the LV
 grid for congestion management. The article describes the
 set-up of the flexibility value chain and shows how all
 individual parts are integrated into the complete process
Titan III Illustrations
Creators: name: Rader And Associates
Year: 1965
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 41
valueUri: https://core.tdar.org/browse/site-name/117500/launch-complex-41
subject: Titan III
valueUri: https://core.tdar.org/browse/other-keyword/164622/titan-iii
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

description: Illustrations of Launch Complex 41.
Site Investigation Report and NFRAP Decision Document for 45th Space Wing at Cape Canaveral Air Station, Florida: Volume 13
Creators: name: O’Brien And Gere Engineers, Inc.
Publisher: name: Air Force Space Command
Year: 1997
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 30
valueUri: https://core.tdar.org/browse/site-name/116306/launch-complex-30
subject: Solid Waste Management Unit# 125
valueUri: https://core.tdar.org/browse/site-name/127656/solid-waste-management-unit-125
subject: SWMU125
valueUri: https://core.tdar.org/browse/site-name/127655/swmu125
subject: L30
valueUri: https://core.tdar.org/browse/site-name/127657/l30
subject: Cape Canaveral Air Force Station
valueUri: https://core.tdar.org/browse/other-keyword/96049/cape-canaveral-air-force-station

description: This document presents the Site Investigation Report and No Further Response Action Planned (NFRAP) Decision Document for 45th Space Wing Facilities at Cape Canaveral Air Station, Launch Complex 30 (L30), Solid Waste Management Unit #125 (SWMU 125) - Revision 1, September 1997.
KIC 3749404: A heartbeat Star with Rapid Apsidal Advance Indicative of a Tertiary Component
Creators: name: Hambleton, Kelly M.
name: Kurtz, Donald W.
name: Prsa, Andrej
name: Quinn, Sam N.
name: Fuller, James
name: Murphy, Simon J.
name: Thompson, Susan E.
name: Latham, David W.
name: Shporer, Avi
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Heartbeat stars are eccentric (e > 0.2) ellipsoidal variables whose light curves resemble a cardiogram. We present the observations and corresponding model of KIC 3749404, a highly eccentric (e = 0.66), short period (P = 20.3 d) heartbeat star with tidally induced pulsations. A binary star model was created using PHOEBE, which we modified to include tidally induced pulsations and Doppler boosting. The morphology of the photometric periastron variation (heartbeat) depends strongly on the eccentricity, inclination and argument of periastron. We show that the inclusion of tidally induced pulsations in the model significantly changes the parameter values, specifically the inclination and those parameters dependent on it. Furthermore, we determine the rate of apsidal advance by modelling the periastron variation at the beginning and end of the 4-yr Kepler data set and dividing by the elapsed time. We compare the model with the theoretical expectations for classical and general relativistic apsidal motion and find the observed rate to be two orders of magnitude greater than the theoretical rate. We find that the observed rate cannot be explained by tidally induced pulsations alone and consequently hypothesise the presence of a third body in the system.
description: 16 pages, 8 figures
Supplementary material for the article "Diagnostic evaluation of institutions as a basis for designing the Brazilian maturity model of telehealth services"
Creators: name: Silva, Angélica Baptista
name: Pisa, Ivan Torres
name: Messina, Luiz Ary
name: Pelogi, Andréa Pereira Simões
name: Tenório, Josceli Maria
name: Sousa, Fernando Sequeira
name: Guedes, Ana Cristina Carneiro Menezes
name: Santos, Daniela Lacerda
name: Maia, Jessi
name: Andrade Filha, Ianê Germano de
name: Lopes, Paulo Roberto de Lima
name: Maia, Paulo Ricardo da Silva
Publisher: name: Zenodo
Year: 2023
Subjects: Telemedicine
Telehealth
Digital Health.
Health Planning

description: Aspects report; Data collection instrument; In-depth interview instructions; and Informed consent document.
An elusive dark central mass in the globular cluster M4
Creators: name: Vitral, Eduardo
name: Libralato, Mattia
name: Kremer, Kyle
name: Mamon, Gary A.
name: Bellini, Andrea
name: Bedin, Luigi R.
name: Anderson, Jay
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Recent studies of nearby globular clusters have discovered excess dark mass in their cores, apparently in an extended distribution, and simulations indicate that this mass is composed mostly of white dwarfs (respectively stellar-mass black holes) in clusters that are core-collapsed (respectively with a flatter core). We perform mass-anisotropy modelling of the closest globular cluster, M4, with intermediate slope for the inner stellar density. We use proper-motion data from Gaia EDR3 and from observations by the Hubble Space Telescope. We extract the mass profile employing Bayesian Jeans modelling, and check our fits with realistic mock data. Our analyses return isotropic motions in the cluster core and tangential motions ($β\approx -0.4$$\pm$$0.1$) in the outskirts. We also robustly measure a dark central mass of roughly $800\pm300 \,$M$_{\odot}$, but it is not possible to distinguish between a point-like source, such as an intermediate-mass black hole (IMBH), or a dark population of stellar remnants of extent $\approx 0.016\,\rm pc \simeq 3300\,AU$. However, when removing a high-velocity star from the cluster centre, the same mass excess is found, but more extended ($\sim 0.034\, \rm{pc} \approx 7000\,\rm AU$). We use Monte Carlo $N$-body models of M4 to interpret the second outcome, and find that our excess mass is not sufficiently extended to be confidently associated with a dark population of remnants. Finally, we discuss the feasibility of these two scenarios (i.e., IMBH vs. remnants), and propose new observations that could help to better grasp the complex dynamics in M4's core.
description: 19 page, 15 figures, 3 tables. Accepted for publication in MNRAS
Launch Complex 37 Maps
Creators: name: Maurice H. Connell & Associates
name: Reynolds, Smith & Mills
Year: 1963
Subjects: subject: Florida (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/2273/florida-state-territory
subject: Cape Canaveral
valueUri: https://core.tdar.org/browse/geographic-keyword/23155/cape-canaveral
subject: Brevard (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/14443/brevard-county
subject: Launch Complex 37
valueUri: https://core.tdar.org/browse/site-name/116301/launch-complex-37
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

description: Maps and Illustrations of Launch Complex 37.
Maps of Roads, Cape Canaveral, Florida
Creators: name: U.S. Army Corps Of Engineers
Year: 1953
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: Road maps
valueUri: https://core.tdar.org/browse/other-keyword/164624/road-maps
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: Records Search / Inventory Checking
valueUri: https://core.tdar.org/browse/investigation-type/8/records-search-inventory-checking

description: Road Maps
Velocity Map Imaging the Scattering Plane of Gas Surface Collisions
Creators: name: Hadden, David J.
name: Messider, Thomas M.
name: Leng, Joseph G.
name: Greaves, Stuart J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The ability of gas-surface dynamics studies to resolve the velocity distribution of the scattered species in the 2D sacattering plane has been limited by technical capabilities and only a few different approaches have been explored in recent years. In comparison, gas-phase scattering studies have been transformed by the near ubiquitous use of velocity map imaging. We describe an innovative means of introducing a surface within the electric field of a typical velocity map imaging experiment. The retention of optimum velocity mapping conditions was demonstrated by measurements of iodomethane-d3 photodissociation and SIMION calculations. To demonstrate the systems capabilities the velocity distributions of ammonia molecules scattered from a PTFE surface have been measured for multiple product rotational states.
description: 8 pages, 5 figures, to be submitted to journal