cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The tuning of para- and diamagnetic cavity photon excitations in a square array of quantum dots in a magnetic field
Creators: name: Gudmundsson, Vidar
name: Mughnetsyan, Vram
name: Goan, Hsi-Sheng
name: Chai, Jeng-Da
name: Abdullah, Nzar Rauf
name: Tang, Chi-Shung
name: Moldoveanu, Valeriu
name: Manolescu, Andrei
Publisher: name: arXiv
Year: 2024
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We employ a ``real-time'' excitation scheme to calculate the excitation spectra of a two-dimensional electron system in a square array of quantum dots placed in a circular cylindrical far-infrared photon cavity subjected to a perpendicular homogeneous external magnetic field. The Coulomb interaction of the electrons is handled via spin density functional theory and the para- and the diamagnetic parts of the electron-photon coupling are updated according to a configuration interaction method in each iteration of the density functional calculation. The results show that an excitation scheme built on using the symmetry of the lateral square superlattice of the dots and the cylindrical cavity produces both para- and diamagnetic resonance peaks with oscillator strengths that can be steered by the excitation pulse parameters. The excitation method breaks the conditions for the generalized Kohn theorem and allows for insight into the subband structure of the electron system and can be used both in and outside the linear response regime.
description: RevTeX - pdfLaTeX, 14 pages with 15 included pdf and png figures
Additional file 1 of Socioeconomic differences in tobacco outlet presence, density, and proximity in four cities in the Netherlands
Creators: name: van Deelen, Tessa R.D.
name: Veldhuizen, Els M.
name: van den Putte, Bas
name: Kunst, Anton E.
name: Kuipers, Mirte A.G.
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences
subject: Computational Biology

description: Supplementary Tables: Supplementary Table 1. Number of neighbourhoods, postcode areas (PC6), and tobacco outlets per city. Supplementary Table 2. Average availability in number, density per km2, and distance in metres tobacco outlets per type of outlet per city (area).
Phytochemicals of Euphorbia tirucalli and their Inhibitory Potential against  Xanthomonas oryzae Ddl Enzyme: An In silico Evaluation for Potential Agrochemical
Creators: name: Miano, John Rowen
Publisher: name: Zenodo
Year: 2024

description: The Bacterial Rice Blight (BRB), caused by the bacteria Xanthomonas oryzae pv. oryzae (Xoo), has had severe global health, social, and economic consequences due to its rapid transmission rate and lack of effective and targeted agricultural interventions. Therefore, there is an urgent need to develop novel anti-BRB repellants and therapeutics. In vitro studies have shown that Euphorbia tirucalli and its bioactive compounds have promising antimicrobial activity. However, their efficacy against the Xanthomonas oryzae Ddl enzyme, a key enzyme that acts as a protective barrier and replicator, is unknown. To address this gap, the researcher used bioinformatics, specifically molecular docking, to dock 8 (eight) phytochemicals from Euphorbia tirucalli onto the Xanthomonas oryzae Ddl enzyme and evaluated their drug-likeness and toxicity risk. The results indicate that Afzelin (4) has a strong binding affinity at -8.0 kcal/mol to the Ddl enzyme and meets the necessary criteria for drug-likeness and toxicity risk. These findings suggest that the plant compound could be a potential candidate for the development of anti-BRB repellants and therapeutics. Further studies are needed to explore its efficacy in vivo and its potential as an agrochemical agent for Bacterial Rice Blight.
Weinmannia magnifolia Cuatrec.
Creators: name: Ulloa Ulloa, Carmen
name: Chaspuengal-Morales, Andrea
name: Fajardo-Gutiérrez, Francisco
name: Oleas, Nora H.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Oxalidales
Cunoniaceae
Weinmannia
Weinmannia magnifolia

description: Weinmannia magnifolia Cuatrec., Caldasia 2: 25, figs. 10 D, 13. 1941.
Type.
Colombia • Dep. de Huila, entre Gabinete y Andalucía, 2300- 2200 m. alt., 24-III-1940, J. Cuatrecasas 8590 (lectotype, designated here: COL [barcode COL 000001498!]; isolectotypes, COL [barcode COL 000001499!], F [barcode F 0063243 F image!], F [barcode F 0063244 F image!], P [barcode P 00697262!], U [barcode U 0082345 image!], US [barcode US 00097274 image!], US [barcode US 00097275 image!]).
Note.
Cuatrecasas (1941) cited a single collection as the type but did not mention the herbarium housing the type (“ Typus: … 24-III-1940, J. Cuatrecasas, 8590. ”). Bernal (2016: 1127) listed the “ isotype ” as (“ IT: COL, F ”). Since there was no holotype, there was no isotype. Although Bernal’s usage of the type term “ isotype ” is correctable to lectotype (see Art. 9.10) his citation of two herbaria and the lack of usage of the phrase “ designated here ” (or its equivalent) do not constitute any inadvertent lectotypification (see Art. 7.11). Furthermore, at COL, we found two duplicates of that collection, and we chose one of them, which agrees well with the protologue, for the lectotypification. This species was accepted in Bernal (2016: 1127).
description: Published as part of Ulloa Ulloa, Carmen, Chaspuengal-Morales, Andrea, Fajardo-Gutiérrez, Francisco & Oleas, Nora H., 2025, Typification of names of Weinmannia (Cunoniaceae) of species described by José Cuatrecasas from Colombian collections, pp. 87-98 in PhytoKeys 254 on pages 87-98, DOI: 10.3897/phytokeys.254.135362
Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
Creators: name: Qin, Ying
name: Zhu, Jin-Ping
name: Meynet, Georges
name: Zhang, Bing
name: Wang, Fa-Yin
name: Shu, Xin-Wen
name: Song, Han-Feng
name: Wang, Yuan-Zhu
name: Yuan, Liang
name: Wang, Zhen-Han-Tao
name: Hu, Rui-Chong
name: Wu, Dong-Hong
name: Yi, Shuang-Xi
name: Tang, Qing-Wen
name: Wei, Jun-Jie
name: Wu, Xue-Feng
name: Liang, En-Wei
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: On April 25th, 2019, the LIGO-Virgo Collaboration discovered a Gravitational-wave (GW) signal from a binary neutron star (BNS) merger, i.e., GW190425. Due to the inferred large total mass, the origin of GW190425 remains unclear. We perform detailed stellar structure and binary evolution calculations that take into account mass-loss, internal differential rotation, and tidal interactions between a He-rich star and a NS companion. We explore the parameter space of the initial binary properties, including initial NS and He-rich masses and initial orbital period. We find that the immediate post-common-envelope progenitor system, consisting of a primary $\sim2.0\,M_\odot$ ($\sim1.7\,M_\odot$) NS and a secondary He-rich star with an initial mass of $\sim3.0-5.5\,M_\odot$ ($\sim5.5-6.0\,M_\odot$) in a close binary with an initial period of $\sim0.08-0.5\,{\rm{days}}$ ($\sim 0.08-0.4\,{\rm{days}}$), that experiences stable Case BB/BC mass transfer (MT) during binary evolution, can reproduce the formation of GW190425-like BNS events. Our studies reveal that the secondary He-rich star of the GW190425's progenitor before its core collapse can be efficiently spun up through tidal interaction, finally remaining as a NS with rotational energy even reaching $\sim10^{52}\,{\rm{erg}}$, which is always much higher than the neutrino-driven energy of the supernova (SN) explosion. If the newborn secondary NS is a magnetar, we expect that GW190425 can be the remnant of a magnetar-driven SN, e.g., a magnetar-driven ultra-stripped SN, a superluminous SN, or a broad-line Type Ic SN. Our results show that GW190425 could be formed through the isolated binary evolution, which involves a stable Case BB/BC MT just after the common envelope phase. On top of that, we show the He-rich star can be tidally spun up, potentially forming a spinning magnetized NS (magnetar) during the second SN explosion.
description: 7 pages, 8 figures, accepted for publication in A&A
Recovering Knowledge from old Code
Creators: name: Erxleben, Fredo
Publisher: name: Zenodo
Year: 2025
Subjects: Reverse Engineering
Legacy Code
FORTRAN 77
Scientific Software
RSE

description: Context

These are the slides for a presentation given at the deRSE'25 conference.

 

Content

The slides cover the topic of approaching the reverse enginnering a scientific legacy code project and outline first steps to take towards unlocking the algorithms therein.
Jüdes, Ulrich, In-vitro-Fertilisation und Embryotransfer (Retortenbaby)
Creators: name: Koltermann, Rainer
Publisher: name: Theologie und Philosophie
Year: 1970

description: Theologie und Philosophie, Bd. 60 Nr. 3 (1985): Theologie und Philosophie, Band 60, Heft 3
Cartan moving frames and the data manifolds
Creators: name: Tron, Eliot
name: Fioresi, Rita
name: Couellan, Nicolas
name: Puechmorel, Stéphane
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: Differential Geometry (math.DG)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: The purpose of this paper is to employ the language of Cartan moving frames to study the geometry of the data manifolds and its Riemannian structure, via the data information metric and its curvature at data points. Using this framework and through experiments, explanations on the response of a neural network are given by pointing out the output classes that are easily reachable from a given input. This emphasizes how the proposed mathematical relationship between the output of the network and the geometry of its inputs can be exploited as an explainable artificial intelligence tool.
Purdue Opinion Panel Poll: Education
Creators: name: Panel, The Purdue Opinion
Publisher: name: Roper Center for Public Opinion Research
Year: 2011

description: Feeling successful (1); basic knowledge acquisition (1); vocational skill training (1); understanding yourself (1); developing physical fitness (1); guidance counselor visits (4); studying drugs (1); dropping out (1); parental school approval (2); teachers' abilities (8); feelings about school (20); school newspaper (1); most important problem (1); government course (1); voter participation (1).
Additional file 3 of Postoperative complications analysis of circular stapled versus linear stapled anastomosis for patients undergoing esophagectomy: a systematic review and meta-analysis
Creators: name: Gu, Hao-Yu
name: Luo, Jing
name: Qiang, Yong
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: Mental Health

description: Additional File 3: PRISMA 2020 Checklist
Non-thermal GeV emission from the Nereides nebula: confirming the nature of the supernova remnant G107.7-5.1
Creators: name: Araya, Miguel
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Recently the Nereides nebula was discovered through deep optical emission line observations and was classified as a supernova remnant (SNR) candidate, G107.7-5.1. Since very little is known about this SNR we look at several archival data sets to better understand the environment and properties of the object. We present a detailed analysis of the gamma-ray emission detected by the \textit{Fermi} Large Area Telescope in the region of the nebula. A model of the non-thermal emission is presented which allows us to derive the particle distribution responsible for the gamma rays. We also use molecular gas and atomic hydrogen observations to try to constrain the source age and distance. An extended (~2deg) GeV source coincident with the location of the nebula is found. The non-thermal emission has a hard spectrum and is detected up to about 100 GeV, confirming the SNR nature of this object. The GeV properties of G107.7-5.1 are similar to those of other SNRs such as G150.3+4.5, and likely expands in a relatively low-density medium. The Nereides nebula is one more example of a growing population of dim SNRs detected at high energies. A simple leptonic model is able to account for the gamma-ray emission. Standard SNR evolutionary models constrain the age to be in the 10-50 kyr range, which is consistent with estimates of the maximum particle energy obtained from GeV observations. However, more detailed observations of the source should be carried out to better understand its properties.
description: Accepted for publication in A&A. 7 pages
Weinmannia myrtifolia Cuatrec.
Creators: name: Ulloa Ulloa, Carmen
name: Chaspuengal-Morales, Andrea
name: Fajardo-Gutiérrez, Francisco
name: Oleas, Nora H.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Oxalidales
Cunoniaceae
Weinmannia
Weinmannia myrtifolia

description: Weinmannia myrtifolia Cuatrec., Caldasia 1 (2): 16, figs. 4, 5 B. 1941.
Type.
Colombia • Cordillera Oriental, vert. oriental, Dep. de Cundinamarca, Bosque en Juiquín, Quebrada Amarilla, bajo el páramo de Guasca, 2840 m. alt., 2-VI-1940, J. Cuatrecasas 9451 (lectotype, designated here, COL [barcode COL 000001501!]; isolectotypes, F [barcode F 0063252 F image!], F [barcode F 0063253 F image!], P [barcode P 02441812!], U [barcode U 0082346 image!], US [barcode US 00097280 image!], US [barcode US 00097281 image!], US [barcode US 00997637 image!]).
Note.
Cuatrecasas (1941) cited a single collection as the type but did not mention the herbarium housing the type (“ Typus: … 2-VI-1940, J. Cuatrecasas, 9451. ”). He also cited a paratype collection as “ Ya en prensa este trabajo, el Dr. A. Dugand ha recolectado en el mismo Páramo de Guasca y en lugar próximo al del tipo unos ejemplares (Dugand 2969: Cordillera oriental: Páramo de Guasca; vertiente oriental, 3100 metros alt., Julio 20, 1941) ”. Bernal (2016: 1126-1127) merely mentioned that the type was housed in COL, F, U, and US herbaria and treated this species as a synonym of W. karsteniana Szyszył. We selected the duplicate deposited at COL as the lectotype.
description: Published as part of Ulloa Ulloa, Carmen, Chaspuengal-Morales, Andrea, Fajardo-Gutiérrez, Francisco & Oleas, Nora H., 2025, Typification of names of Weinmannia (Cunoniaceae) of species described by José Cuatrecasas from Colombian collections, pp. 87-98 in PhytoKeys 254 on pages 87-98, DOI: 10.3897/phytokeys.254.135362
The observational evidence that all microflares that accelerate electrons to high energies are rooted in sunspots
Creators: name: Battaglia, Andrea Francesco
name: Krucker, Säm
name: Veronig, Astrid M.
name: Stiefel, Muriel Zoë
name: Warmuth, Alexander
name: Benz, Arnold O.
name: Ryan, Daniel F.
name: Collier, Hannah
name: Harra, Louise
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In general, large solar flares are more efficient at accelerating high-energy electrons than microflares. Nonetheless, we sometimes observe microflares that accelerate electrons to high energies. We statistically characterize 39 microflares with strikingly hard spectra in the hard X-ray (HXR) range, which means that they are efficient in accelerating high-energy electrons. We refer to these events as "hard microflares." The statistical analysis is built upon spectral and imaging information from STIX, combined with EUV and magnetic field maps from SDO. The key observational result is that all hard microflares in this dataset have one of the footpoints rooted directly within a sunspot (either in the umbra or the penumbra). This clearly indicates that the underlying magnetic flux densities are large. For the events with the classic two-footpoints morphology, the absolute value of the mean line-of-sight magnetic flux density (and vector magnetic field strength) at the footpoint rooted within the sunspot ranges from 600 to 1800 G (1500 to 2500 G), whereas the outer footpoint measures from 10 to 200 G (100 to 400 G), therefore about 10 times weaker. Approximately 78% of hard microflares, which exhibited two HXR footpoints, have similar or even stronger HXR flux from the footpoint rooted within the sunspot. This contradicts the magnetic mirroring scenario. In addition, about 74% of the events could be approximated by a single loop geometry, demonstrating that hard microflares typically have a relatively simple morphology. We conclude that all hard microflares are rooted in sunspots, which implies that the magnetic field strength plays a key role in efficiently accelerating high-energy electrons, with hard HXR spectra associated with strong fields. This key result will allow us to further constrain our understanding of the electron acceleration mechanisms in flares and space plasmas.
description: Accepted for publication in A&A. 16 pages, 11 figures
Roper Commercial # 32: Louisville II -- Public Schools
Creators: name: Organization, The Roper
Publisher: name: Roper Center for Public Opinion Research
Year: 2019

description: Public school rating (1); Louisville public school comparison (1); hobbies (15); night school subjects (15); increased school taxes (1); University of Louisville tax collection (6); last grade of school (2); most valuable subject studied (1); college courses (3); children in school (2); children attending college (6); gendered schools (1); sex education (1); public library card (3); teen-age clubs (2); radio ownership (2).
Rhode Island Poll: 2000 Election/Clinton/Brown Community Learning
Creators: name: Center For Public Policy, Brown University
Publisher: name: Roper Center for Public Opinion Research
Year: 2014

description: Economy (6); important problem (1); voting intention (1); Monica Lewinsky affair (4); Monica Clinton (1); blood-alcohol (1); smoking (1); Brown Learning Community (1); college (5); Brown (2); job performance of Rhode Island political leaders (11).
Additional file 1 of The impact of glucagon-like peptide-1 receptor agonists in the patients undergoing anesthesia or sedation: systematic review and meta-analysis
Creators: name: do Nascimento, Tatiana S.
name: Pereira, Rodrigo O. L.
name: Maia, Eduardo
name: Ohnuma, Tetsu
name: da Costa, Mariana G.
name: Slawka, Eric
name: Galhardo, Carlos
name: Krishnamoorthy, Vijay
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Mental Health

description: Supplementary Material 1. Supplementary figure: Figure S1. Quality assessment.
Additional file 1 of Evaluating construct validity of computable acute respiratory distress syndrome definitions in adults hospitalized with COVID-19: an electronic health records based approach
Creators: name: Sathe, Neha A.
name: Xian, Su
name: Mabrey, F. Linzee
name: Crosslin, David R.
name: Mooney, Sean D.
name: Morrell, Eric D.
name: Lybarger, Kevin
name: Yetisgen, Meliha
name: Jarvik, Gail P.
name: Bhatraju, Pavan K.
name: Wurfel, Mark M.
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Supplementary Material 1
A NICER View of PSR J1231$-$1411: A Complex Case
Creators: name: Salmi, Tuomo
name: Deneva, Julia S.
name: Ray, Paul S.
name: Watts, Anna L.
name: Choudhury, Devarshi
name: Kini, Yves
name: Vinciguerra, Serena
name: Cromartie, H. Thankful
name: Wolff, Michael T.
name: Arzoumanian, Zaven
name: Bogdanov, Slavko
name: Gendreau, Keith
name: Guillot, Sebastien
name: Ho, Wynn C. G.
name: Morsink, Sharon M.
name: Cognard, Ismaël
name: Guillemot, Lucas
name: Theureau, Gilles
name: Kerr, Matthew
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recent constraints on neutron star mass and radius have advanced our understanding of the equation of state (EOS) of cold dense matter. Some of them have been obtained by modeling the pulses of three millisecond X-ray pulsars observed by the Neutron Star Interior Composition Explorer (NICER). Here, we present a Bayesian parameter inference for a fourth pulsar, PSR J1231$-$1411, using the same technique with NICER and XMM-Newton data. When applying a broad mass-inclination prior from radio timing measurements and the emission region geometry model that can best explain the data, we find likely converged results only when using a limited radius prior. If limiting the radius to be consistent with the previous observational constraints and EOS analyses, we infer the radius to be $12.6 \pm 0.3$ km and the mass to be $1.04_{-0.03}^{+0.05}$ $M_\odot$, each reported as the posterior credible interval bounded by the $16\,\%$ and $84\,\%$ quantiles. If using an uninformative prior but limited between $10$ and $14$ km, we find otherwise similar results, but $R_{\mathrm{eq}} = 13.5_{-0.5}^{+0.3}$ km for the radius. In both cases, we find a nonantipodal hot region geometry where one emitting spot is at the equator or slightly above, surrounded by a large colder region, and where a noncircular hot region lies close to southern rotational pole. If using a wider radius prior, we only find solutions that fit the data significantly worse. We discuss the challenges in finding the better fitting solutions, possibly related to the weak interpulse feature in the pulse profile.
description: 23 pages, 13 figures (2 of which are figure sets), 3 tables, published in ApJ
Indications of magnetic accretion in Swift J0826.2-7033
Creators: name: Rawat, Nikita
name: De Martino, Domitilla
name: Mukai, Koji
name: Falanga, Maurizio
name: Masetti, Nicola
name: Pandey, Jeewan C.
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present our findings from the first long X-ray observation of the hard X-ray source Swift J0826.2-7033 with XMM-Newton, which has shown characteristics of magnetic accretion. The system appears to have a long orbital period (~7.8 h) accompanied by short timescale variabilities, which we tentatively interpret as the spin and beat periods of an intermediate polar. These short- and long-timescale modulations are energy-independent, suggesting that photoelectric absorption does not play any role in producing the variabilities. If our suspected spin and beat periods are true, then Swift J0826.2-7033 accretes via disc-overflow with an equal fraction of accretion taking place via disc and stream. The XMM-Newton and Swift-BAT spectral analysis reveals that the post-shock region in Swift J0826.2-7033 has a multi-temperature structure with a maximum temperature of ~43 keV, which is absorbed by a material with an average equivalent hydrogen column density of ~1.6$\times$10$^{22}$ cm$^{-2}$ that partially covers ~27% of the X-ray source. The suprasolar abundances, with hints of an evolved donor, collectively make Swift J0826.2-7033 an interesting target, which likely underwent a thermal timescale mass transfer phase.
description: 10 pages, 7 figures. Accepted for publication in A&A
Additional file 2 of Altitude-dependent agro-ecologies impact the microbiome diversity of scavenging indigenous chicken in Ethiopia
Creators: name: Glendinning, Laura
name: Jia, Xinzheng
name: Kebede, Adebabay
name: Oyola, Samuel O.
name: Park, Jong-Eun
name: Park, Woncheoul
name: Assiri, Abdulwahab
name: Holm, Jacob Bak
name: Kristiansen, Karsten
name: Han, Jianlin
name: Hanotte, Olivier
Publisher: name: figshare
Year: 2024
Subjects: subject: Space Science
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified

description: Additional file 2: Supplementary Results 1. Detection of slow-growing microbes: Fig. S1. Boxplot showing the predicted doubling time of strain-level MAGs, by phylum. The red, dashed line indicates the cut-off point above which MAGs are considered oligotrophs. Fig. S2. Growth rate distributions for strain-level genomes from MAGs produced in this study (Current_MAGs: 9977) and dereplicated genomes from the NSC dataset, which originated from cultured isolates (NSC_cultured: 170) or were MAGs (NSC_MAGs: 2343). The red, dashed line indicates the cut-off point above which MAGs are considered oligotrophs. Relating CAZyme abundance to oligotrophy: Fig. S3. Total CAZyme families count vs maximal growth rate. A) Unique CAZyme families, B) Total CAZyme genes. The red, dashed line indicates the cut-off point above which MAGs are considered oligotrophs. Copiotrophs were found to have significantly more CAZyme genes and unique CAZyme families than oligotrophs (Kruskal-Wallis: P<2.2e-16).
sj-docx-2-aas-10.1177_00953997221109308 – Supplemental material for Learning and Adaptation in Polycentric Transport Governance: The Case of the Dutch Brabant Accessibility Agenda
Creators: name: Van Assche, Kristof
name: Beunen, Raoul
name: Verweij, Stefan
name: Evans, Joshua
name: Gruezmacher, Monica
name: Bousema, Ingo
name: Busscher, Tim
name: Rauws, Ward
name: Leendertse, Wim
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 160607 International Relations
subject: FOS: Political science
subject: 160509 Public Administration

description: Supplemental material, sj-docx-2-aas-10.1177_00953997221109308 for Learning and Adaptation in Polycentric Transport Governance: The Case of the Dutch Brabant Accessibility Agenda by Ingo Bousema, Tim Busscher, Ward Rauws and Wim Leendertse in Administration & Society
Global-TRANSIT: modeling global historic sailing using a least-cost surface analysis
Creators: name: Roberts, Lucinda
name: Merson, Joanna
name: Wong, Woan Foong
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Neuroscience
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Cost-surface analyses in geographic information systems (GIS) can be a useful tool for approximating the travel of historic sailing ships to fill gaps in the historic record. We present the Global-TRANSIT workflow, a least-cost surface raster analysis that uses wind speed and direction to estimate sailing routes and durations for ports globally. Our workflow, freely available as a Python notebook for ArcGIS Pro, makes three contributions relative to previously published toolkits. First, our workflow estimates sail travel for ports at the global scale while accounting for projection-related challenges. Second, our workflow evaluates origin and destination pairs in a many-origins-to-many-destinations matrix structure (compared to previous one-origin-to-one-destination relationship) which increases the scalability of our toolbox. Third, our workflow replaces the deprecated tools used in the previous work with newer tools that reduce the grid-induced bias. Despite the expected limitations of modeling a complex phenomenon like sailing, we find a high correlation between our modeled estimates and historically observed sail duration and routes. The outputs of Global-TRANSIT provide an approximation of the likely duration and route of sail travel between worldwide ports, serving as a reference for understanding historic sail voyage patterns globally and as a benchmark for measuring the evolution of maritime shipping over time.
Siena Research Institute Poll: January 2011 Siena New York State Consumer Confidence Index
Creators: name: Siena Research Institute, Siena College
Publisher: name: Roper Center for Public Opinion Research
Year: 2012

description: Financial situation (2); New York business conditions (1); New York future economic situation (1); good time to buy (1); future purchases (5); effects of gas prices (1); effects of food prices (1); real estate improvements (2); selling property (2); buying property (2).
Weinmannia ovalis var. petiolata Cuatrec.
Creators: name: Ulloa Ulloa, Carmen
name: Chaspuengal-Morales, Andrea
name: Fajardo-Gutiérrez, Francisco
name: Oleas, Nora H.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Oxalidales
Cunoniaceae
Weinmannia
Weinmannia ovalis
Weinmannia ovalis ruiz & pav. var. petiolata cuatrec.

description: Weinmannia ovalis Ruiz & Pav. var. petiolata Cuatrec., Lloydia 11 (3): 203. 1948 [1949].
Type.
Colombia • Dep. del Valle, Cordillera Occidental, Los Farallones, Quebrada de Las Nieves, lomas parameras sobre la mina El Diamante 3100–3120 m, 31-VII-1946, J. Cuatrecasas 21820 (lectotype, designated here: F [barcode V 0334900 F image!]; isolectotypes, F [barcode V 0334901 F image!], COL [barcode COL 000076221!], P [P 05518589 image!]).
Note.
Cuatrecasas (1948 [1949]) did cite the collection J. Cuatrecasas 21820 housed at the F Herbarium as the type; however, in the F Herbarium there are two duplicates of the collection, and both specimens lack the holotype annotation, and thus constitute syntypes; we chose one of them for the lectotypification (cf. Art. 40 Ex. 3). This variety is a synonym of W. elliptica Kunth according to Bernal (2016: 1126).
description: Published as part of Ulloa Ulloa, Carmen, Chaspuengal-Morales, Andrea, Fajardo-Gutiérrez, Francisco & Oleas, Nora H., 2025, Typification of names of Weinmannia (Cunoniaceae) of species described by José Cuatrecasas from Colombian collections, pp. 87-98 in PhytoKeys 254 on pages 87-98, DOI: 10.3897/phytokeys.254.135362
title: Climatic and Ecological Change in the Americas
title: Reseña de libro
titleType: AlternativeTitle
Creators: name: Kirmes, Eva Sophia
Publisher: name: Abteilung für Altamerikanistik, Universität Bonn
Year: 2024
Subjects: subject: climate change
subject: ecological change
subject: Americas
subject: ddc:300
subject: ddc:333.7
subject: ddc:980

description: Reseña de libro / Review of the book:
 Whitaker, Armstrong & Odonne (eds.): Climatic and Ecological Change in the Americas : A Perspective from Historical Ecology, 2023. London: Routdlege, 256 p., ISBN: 9781003316497, Open Access.
The Multi-Epoch Jet Outbursts in Abell 496: synchrotron ageing and buoyant X-ray cavities draped by warm gas filaments
Creators: name: Ubertosi, Francesco
name: Giacintucci, Simona
name: Clarke, Tracy
name: Markevitch, Maxim
name: Venturi, Tiziana
name: O'Sullivan, Ewan
name: Gitti, Myriam
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The galaxy cluster Abell 496 has been extensively studied in the past for the clear sloshing motion of the hot gas on large scales, but the interplay between the central radio galaxy and the surrounding cluster atmosphere is mostly unexplored. We present a dedicated radio, X-ray, and optical study of Abell 496 aimed at investigating this connection. We use deep radio images obtained with the Giant Metrewave Radio Telescope at 150, 330 and 617 MHz, Very Large Array at 1.4 and 4.8 GHz, and VLA Low Band Ionosphere and Transient Experiment at 340 MHz, with angular resolutions ranging from 0.''5 to 25''. Additionally, we use archival Chandra and Very Large Telescope MUSE observations. The radio images reveal three distinct periods of jet activity: an ongoing episode on sub-kpc scales with an inverted radio spectrum; an older episode that produced lobes on scales $\sim$20 kpc which now have a steep spectral index ($α= 2.0 \pm 0.1$); and an oldest episode that produced lobes on scales of $\sim$50 - 100 kpc with an ultra-steep spectrum ($α= 2.7 \pm 0.2$). Archival Chandra X-ray observations show that the older and oldest episodes have excavated two generations of cavities in the hot gas of the cluster. The outermost X-ray cavity has a clear mushroom-head shape, likely caused by its buoyant rise in the cluster's potential. Cooling of the hot gas is ongoing in the innermost 20 kpc, where H$α$-bright warm filaments are visible in VLT-MUSE data. The H$α$-filaments are stretched towards the mushroom-head cavity, which may have stimulated ICM cooling in its wake. We conclude by commenting on the non-detection of a radio mini-halo in this vigorously sloshing, but low-mass, galaxy cluster.
description: Accepted for publication in Astronomy & Astrophysics
Siena Research Institute Poll: May 2016 Siena New York Poll
Creators: name: Siena Research Institute, Siena College
Publisher: name: Roper Center for Public Opinion Research
Year: 2016

description: Direction of New York State (1); direction of country (1); opinion of people and institutions in public life (9); 2016 election for U.S. Senator (1); 2016 election for President (1); Hillary Clinton vs. Donald Trump (1); vote to re-elect Governor Andrew Cuomo (1); Andrew Cuomo job performance as Governor (1); Andrew Cuomo policies as ethical or not (1); preferred political party to control State Senate (1); important issues for Governor and State Legislature to act on (7); corruption in state government (4); view on State Legislature becoming full-time with outside employment banned (1); how will recent corruption scandals affect your vote to re-elect state legislators (2); optimism that the Governor and Legislature will enact anti-corruption legislation (1); support or oppose ride sharing companies, Uber (1); legalize daily fantasy sports companies, FanDuel/Draftkings (1).
Brandenstein, Bela Freiherr von, "Sein - Welt - Mensch"
Creators: name: Cooper, B. Dehmelt
Publisher: name: Theologie und Philosophie
Year: 1970

description: Theologie und Philosophie, Bd. 60 Nr. 3 (1985): Theologie und Philosophie, Band 60, Heft 3
Weinmannia parvifoliolata Cuatrec.
Creators: name: Ulloa Ulloa, Carmen
name: Chaspuengal-Morales, Andrea
name: Fajardo-Gutiérrez, Francisco
name: Oleas, Nora H.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Oxalidales
Cunoniaceae
Weinmannia
Weinmannia parvifoliolata

description: Weinmannia parvifoliolata Cuatrec., Caldasia 2: 21, figs. 9, 10 A. 1941.
Type.
Colombia • Cordillera Oriental de Colombia, en el filo divisorio entre la Comisaría del Caquetá y Departamento del Huila, 2300–2400 m. alt., 22-III-1940, J. Cuatrecasas 8486 - A (lectotype, designated by Bernardi (1961: 147): F [barcode F 0063261 F image!], isolectotypes: COL [barcode COL 000001502!]; US [barcode US 00097286 image!], US [barcode US 00997638 image!]).
Note.
Although Cuatrecasas (1941) cited a single collection as the type, he did not mention the herbarium housing the type (“ Typus: … 22-III-1940, J. Cuatrecasas, 8496 - A. ”). Bernardi (1961: 147) assumed that the holotype was at the COL Herbarium and mentioned the duplicate at the F Herbarium as an “ isotype ”. Since there was no holotype, there was no isotype, nonetheless, Bernardi’s usage of the type term “ isotype ” is correctable to lectotype (see Art. 9.10). Therefore, Bernardi’s citation of “ isotype ” is treated here as the inadvertent lectotype designation; Bernal (2016: 1127) merely mentioned the isotype (“ IT: COL, F ”) and accepted this species.
description: Published as part of Ulloa Ulloa, Carmen, Chaspuengal-Morales, Andrea, Fajardo-Gutiérrez, Francisco & Oleas, Nora H., 2025, Typification of names of Weinmannia (Cunoniaceae) of species described by José Cuatrecasas from Colombian collections, pp. 87-98 in PhytoKeys 254 on pages 87-98, DOI: 10.3897/phytokeys.254.135362
CHANG-ES XXXIV: a 20 kpc radio bubble in the halo of the star-forming galaxy NGC 4217
Creators: name: Heesen, V.
name: Wiegert, T.
name: Irwin, J.
name: Crocker, R.
name: Kiehn, A.
name: Li, J. -T.
name: Wang, Q. D.
name: Stein, M.
name: Dettmar, R. -J.
name: Soida, M.
name: Henriksen, R.
name: Gajovic, L.
name: Yang, Y.
name: Brüggen, M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Cosmic rays may be dynamically very important in driving large-scale galactic winds. Edge-on galaxies give us an outsider's view of the radio halo, which shows the presence of extra-planar cosmic-ray electrons and magnetic fields. We present a new radio continuum imaging study of the nearby edge-on galaxy NGC 4217 in order to study the distribution of extra-planar cosmic rays and magnetic fields. We both observe with the Jansky Very Large Array (JVLA) in the S-band (2-4 GHz) and with LOw Frequency ARray (LOFAR) at 144 MHz. We measure vertical intensity profiles and exponential scale heights. We re-image both JVLA and LOFAR data at matched angular resolution in order to measure radio spectral indices between 144 MHz and 3 GHz. Confusing point-like sources were subtracted prior to imaging. Intensity profiles are then fitted with cosmic-ray electron advection models, where we use an isothermal wind model that is driven by a combination of pressure from the hot gas and cosmic rays. We discover a large-scale radio halo on one (northwestern) side of the galactic disc. The morphology is reminiscent of a bubble extending up to 20 kpc away from the disc. We find spectral ageing in the bubble which allows us to measure advection speeds of the cosmic-ray electrons accelerating from 300 to 600 $\rm km\, s^{-1}$ . Assuming energy equipartition between the cosmic rays and the magnetic field, we estimate the bubble can be inflated by a modest 10 per cent of the kinetic energy injected by supernovae over its dynamical time-scale of 35 Myr. While no active galactic nucleus (AGN) has been detected, such activity in the recent past cannot be ruled out. Non-thermal bubbles with sizes of tens of kiloparsec may be a ubiquitous feature of star-forming galaxies showing the influence of feedback. To determine possible contributions by AGN feedback, will require deeper observations.
description: Accepted to Astronomy and Astrophysics. 9 pages, 7 figures, 1 table
Additional file 1 of Evaluating effectiveness of screening house eaves as a potential intervention for reducing indoor vector densities and malaria prevalence in Nyabondo, western Kenya
Creators: name: Ng’ang’a, Peter Njoroge
name: Collins Okoyo
name: Mbogo, Charles
name: Mutero, Clifford Maina
Publisher: name: figshare
Year: 2020
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. Number of indoor adult mosquitoes collected in Nyabondo for two years, separated by species and the study arm.
Deformations of the AdS-Schwarzschild black brane and the shear viscosity of the quark-gluon plasma
Creators: name: da Rocha, Roldao
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Deformations of the AdS$_5$-Schwarzschild black brane, implemented in the AdS/CFT membrane paradigm, are scrutinized in the dual viscous hydrodynamic infrared limit. The latest experimental data analyses, regarding the shear viscosity-to-entropy density ratio of the quark-gluon plasma produced by heavy-ion collisions at the LHC and RHIC, are shown to constrain these deformations severely. Although corroborating with the robustness of the standard AdS$_5$-Schwarzschild black brane against deformations, there is still a margin for mild deformations which may carry 2-loop quantum corrections to gravity, whose implications to the strongly-coupled dual field theory are addressed and discussed.
description: 42 pages, 8 figures
sj-docx-2-jad-10.1177_10870547221106238 – Supplemental material for Analysis of Daily Sleep Diary Measures From Multilayer Extended-Release Methylphenidate (PRC-063) Studies in Children and Adults With ADHD
Creators: name: Cataldo, Marc
name: Donnelly, Graeme
name: Cutler, Andrew J.
name: Childress, Ann
name: Mikl, Jaromir
name: Bhaskar, Sailaja
name: Waxmonsky, James
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: Education
subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Supplemental material, sj-docx-2-jad-10.1177_10870547221106238 for Analysis of Daily Sleep Diary Measures From Multilayer Extended-Release Methylphenidate (PRC-063) Studies in Children and Adults With ADHD by Marc Cataldo, Graeme Donnelly, Andrew J. Cutler, Ann Childress, Jaromir Mikl, Sailaja Bhaskar and James Waxmonsky in Journal of Attention Disorders
Nikkei Research Poll: November 2006
Creators: name: Nikkei Research, Inc.
Publisher: name: Roper Center for Public Opinion Research
Year: 2013

description: Support for Shinzo Abe's Cabinet (1); reason for supporting Abe Cabinet (1); reason for not supporting Abe Cabinet (1); political party preference (2); Abe priority (1); Abe reformation attitude (1); Liberal Democratic Party of Japan accepting rebellion members (1); influence of rebellion members (1); limitations after corruption cases (1); education reform law (1); stronger ally (1).
Advanced Classification of Hot Subdwarf Binaries Using Artificial Intelligence Techniques and Gaia DR3 data
Creators: name: Vázquez, C. Viscasillas
name: Solano, E.
name: Ulla, A.
name: Ambrosch, M.
name: Álvarez, M. A.
name: Manteiga, M.
name: Magrini, L.
name: Santoveña-Gómez, R.
name: Dafonte, C.
name: Pérez-Fernández, E.
name: Aller, A.
name: Drazdauskas, A.
name: Mikolaitis, Š.
name: Rodrigo, C.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Hot subdwarfs are compact blue evolved objects, burning helium in their cores surrounded by a tiny hydrogen envelope. Most models agree on a common envelope binary evolution scenario in the Red Giant phase. However, the binarity rate for these objects is yet unsolved. We aim to develop a novel classification method for identifying hot subdwarf binaries within large datasets using Artificial Intelligence methods and Gaia DR3 data. The results will be compared with those obtained previously using VOSA (Virtual Observatory Sed Analyzer) on coincident samples. The methods include several machine learning techniques. We used Support Vector Machines (SVM) to classify 3084 hot subdwarf stars based on their color-magnitude properties. Of these, 2815 objects have Gaia Data Release 3 BP/RP spectra, which were classified using Self-Organizing Maps (SOM) and Convolutional Neural Networks (CNN). The findings demonstrate a high agreement level (70-90%) with VOSA's classification, indicating that machine learning methods effectively classify sources with an accuracy comparable to human inspection or non-AI techniques. SVM in a radial basis function achieves 70.97% reproducibility for binary targets using photometry. CNN reaches 84.94% for binary detection using spectroscopy. We also found that the single-binary differences are especially observable on the infrared flux in our GDR3 BP/BR spectra, at wavelengths larger than 700 nm. We found that all our methods are effective in discerning between single and binary systems and are consistent with the results previously obtained with VOSA. In global terms, considering all quality metrics, CNN is the method that provides the best accuracy. The methods are also effective for detecting peculiarities in the spectra. Further research is needed to refine our techniques and enhance automated classification reliability, especially for large-scale surveys.
Weinmannia penicillata Cuatrec.
Creators: name: Ulloa Ulloa, Carmen
name: Chaspuengal-Morales, Andrea
name: Fajardo-Gutiérrez, Francisco
name: Oleas, Nora H.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Oxalidales
Cunoniaceae
Weinmannia
Weinmannia penicillata

description: Weinmannia penicillata Cuatrec., Caldasia 2: 13, figs. 1, 2. 1941.
≡ W. ovalis var. penicillata (Cuatrec.) Cuatrec., Lloydia 11 (3): 203. 1948 [1949].
Type.
Colombia • Cordillera Oriental sobre el filo divisorio entre el Dept. del Huila y la Comisaría del Caquetá, en Gabinete, 2300-2450 m alt., 21-III-1940, J. Cuatrecasas 8430 (lectotype, designated here, F [barcode F 0063264 F image!]; isolectotypes, CM [barcode CM 0754 image!], COL [barcode COL 000001503!], F [barcode F 0063263 F image!], G [barcode G 00357648 (fragment) image!], US [barcode US 00097287 image!]).
Note.
Cuatrecasas (1941) cited a single collection as the type but he did not mention the herbarium housing it (“ Typus: … 21-III-1940, J. Cuatrecasas, 8430. ”). Subsequently, he mentioned (Cuatrecasas 1948 [1949]) that the type was housed in the F Herbarium. We, however, found two duplicates of that collection at F. Therefore, it is interpreted that Cuatrecasas (1948 [1949]) inadvertently did the first-step lectotypification process, and we herewith do the second-step lectotypification process. Bernal (2016: 1126) treated this species as a synonym of W. elliptica Kunth.
description: Published as part of Ulloa Ulloa, Carmen, Chaspuengal-Morales, Andrea, Fajardo-Gutiérrez, Francisco & Oleas, Nora H., 2025, Typification of names of Weinmannia (Cunoniaceae) of species described by José Cuatrecasas from Colombian collections, pp. 87-98 in PhytoKeys 254 on pages 87-98, DOI: 10.3897/phytokeys.254.135362
Connecticut Poll # 92
Creators: name: Courant, The Hartford
Publisher: name: Roper Center for Public Opinion Research
Year: 2019

description: George Bush job performance (1); concerns about environmental problems (1); Exxon/Alaskan oil spill (12); exploring for oil in wilderness areas (7); mother's family ties (5); family roles of husband and wife (15); motherhood vs. career (6); William O'Neill/General Assembly job performance (2); state budget problems (4); Long Island Sound (9); party identification (1); integration of schools/busing (7); ideology (1).
Additional file 1 of ggcoverage: an R package to visualize and annotate genome coverage for various NGS data
Creators: name: Song, Yabing
name: Wang, Jianbin
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Additional figures. Fig. S1. Three styles of genome coverage plot. Fig. S2. Highlight SNV with three styles. Fig. S3. Protein coverage plot based on peptides obtained by mass spectrometry and annotation of protein characteristics. Fig. S4. Examples of figure customization.
Priority list of root/rhizosphere ideotype traits Summary (Deliverable 1.1)
Creators: name: White, Charlotte
name: Berry, Pete
Publisher: name: Zenodo
Year: 2023
Subjects: Root2ResDeliverable
Root
Root2Res
Rhizosphere
Ideotypes
Roottraits

description: The aim of this document is to ascertain which below ground crop traits confer tolerance against water and phosphorus stress and therefore which traits are likely to be involved in resilience to environmental change.
Additional file 2 of ggcoverage: an R package to visualize and annotate genome coverage for various NGS data
Creators: name: Song, Yabing
name: Wang, Jianbin
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2. The codes used to generate the figures without typesetting for Fig. 1.