cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of Allergy-related diseases in childhood and risk for abdominal pain-related functional gastrointestinal disorders at 16 years—a birth cohort study
Creators: name: Sjölund, Jessica
name: Kull, Inger
name: Bergström, Anna
name: Järås, Jacob
name: Ludvigsson, Jonas F.
name: Törnblom, Hans
name: Simrén, Magnus
name: Olén, Ola
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Cell Biology
Biotechnology
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Science Policy

description: Additional file 1. Age-specific definitions of asthma, rhinitis, eczema, and food hypersensitivity and questionnaire questions used for classification of food hypersensitivity.
The Stellar Mass Spectrum in the Young Populous Cluster NGC 1866
Creators: name: Bergh, Sidney van den
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The young populous cluster NGC 1866 in the Large Magellanic Cloud LMC), which is probably one of the most massive object formed in the LMC during the last ~ 3 Gyr, appears to have an unexpectedly high mass-to-light ratio. From its velocity dispersion Fischer et al. (1992) find its mass to be (1.35 " 0.25) x 105 Mu. The luminosity of this cluster is MV = -8.93 " 0.13, corresponding to LV = (3.2 " 0.4) x 105 LV (u). This yields M/LV = 0.42 " 0.09 in solar units. For a cluster of age 0.1 Gyr such a relatively high mass-to-light ratio requires a mass spectrum with an exponent x = 1.72 " 0.09; or x = 1.75 " 0.09 if mass loss by evolving stars is taken into account.
description: To be published in the October 1999 issue of the Publications of the Astronomical Society of the Pacific
Fusing Individualized Treatment Rules Using Secondary Outcomes
Creators: name: Gao, Daiqi
name: Wang, Yuanjia
name: Zeng, Donglin
Publisher: name: arXiv
Year: 2024
Subjects: subject: Methodology (stat.ME)
subject: Applications (stat.AP)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: An individualized treatment rule (ITR) is a decision rule that recommends treatments for patients based on their individual feature variables. In many practices, the ideal ITR for the primary outcome is also expected to cause minimal harm to other secondary outcomes. Therefore, our objective is to learn an ITR that not only maximizes the value function for the primary outcome, but also approximates the optimal rule for the secondary outcomes as closely as possible. To achieve this goal, we introduce a fusion penalty to encourage the ITRs based on different outcomes to yield similar recommendations. Two algorithms are proposed to estimate the ITR using surrogate loss functions. We prove that the agreement rate between the estimated ITR of the primary outcome and the optimal ITRs of the secondary outcomes converges to the true agreement rate faster than if the secondary outcomes are not taken into consideration. Furthermore, we derive the non-asymptotic properties of the value function and misclassification rate for the proposed method. Finally, simulation studies and a real data example are used to demonstrate the finite-sample performance of the proposed method.
Variable stars in the field of the open cluster NGC 7789
Creators: name: Mochejska, B. J.
name: Kaluzny, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of our search for variable stars in the intermediate-age open cluster NGC 7789. We have found 45 variable stars: 35 eclipsing binaries, five pulsating variables and five miscellaneous variables. Most of the eclipsing binaries show W UMa type of variability, with periods shorter than one day. Four systems exhibit unusual behavior: two, V4276 and V6698, are probably RS CVn stars, another, V3283, is a possible cataclysmic binary. The nature of the fourth binary, V2130, is unclear: the system exhibits assymetric maxima. Among the pulsating variables two, V3407C and V4805 are background RR Lyrae stars and one, V6736, is a delta Scuti variable which is a blue straggler belonging to the cluster. Some of the miscellaneous variables may have periods longer than the five day timespan of our observations. We also present a color-magnitude diagram for the NGC 7789 open cluster, fairly complete down to V ~ 20. The relatively large number of variables found in the comparison field (14 compared to 31 in the cluster field) implies that objects not associated physically with the cluster can account for a significant number of variables identified in the cluster field, as well as in other globular and open clusters observed on a dense background/foreground of disk stars.
description: 23 pages, LaTeX, 10 Postscript figures, submitted to Acta Astronomica
Literature Review for the Paradise Wildfire Resilience Project
Creators: name: DiPietro, Deanne
name: D. Syphard, Alexandra
name: Spencer, Wayne
name: Rustigian-Romsos, Heather
name: Barnard, Phoebe
name: Joseph, Gladwin
Publisher: name: figshare
Year: 2021
Subjects: subject: 129999 Built Environment and Design not elsewhere classified
subject: FOS: Civil engineering
subject: 50202 Conservation and Biodiversity
subject: FOS: Biological sciences
subject: 120501 Community Planning
subject: FOS: Social and economic geography

description: As part of the project “Nature-Based Wildfire Resilience in Paradise, California,” Conservation Biology Institute produced this review and summary of the most recent scientific research describing fire behavior in relation to land use patterns. The overarching objective of the review is to summarize relevant literature to determine how structure loss or other metrics of human impacts are affected by community design, and especially how buffering communities with lower-flammability land uses (e.g., green spaces or agriculture) could potentially reduce structure loss and simultaneously protect natural areas from human impacts. Specifically, we assemble information that could help determine: ● how greenbelts have the potential to mitigate wildfire impacts on California’s communities, and inversely, community impacts on wildlands; ● relevant design elements or parameters such as buffer width, composition, or management that affect wildfire risks in differing ecological contexts; ● key uncertainties or data gaps for the efficacy of using natural, semi-natural, or human-created land uses to minimize wildfire risk to communities.
MUSTARD: Mastering Uniform Synthesis of Theorem and Proof Data
Creators: name: Huang, Yinya
name: Lin, Xiaohan
name: Liu, Zhengying
name: Cao, Qingxing
name: Xin, Huajian
name: Wang, Haiming
name: Li, Zhenguo
name: Song, Linqi
name: Liang, Xiaodan
Publisher: name: arXiv
Year: 2024
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Computation and Language (cs.CL)
subject: Formal Languages and Automata Theory (cs.FL)
subject: Machine Learning (cs.LG)
subject: Programming Languages (cs.PL)
subject: FOS: Computer and information sciences

description: Recent large language models (LLMs) have witnessed significant advancement in various tasks, including mathematical reasoning and theorem proving. As these two tasks require strict and formal multi-step inference, they are appealing domains for exploring the reasoning ability of LLMs but still face important challenges. Previous studies such as Chain-of-Thought (CoT) have revealed the effectiveness of intermediate steps guidance. However, such step-wise annotation requires heavy labor, leading to insufficient training steps for current benchmarks. To fill this gap, this work introduces MUSTARD, a data generation framework that masters uniform synthesis of theorem and proof data of high quality and diversity. MUSTARD synthesizes data in three stages: (1) It samples a few mathematical concept seeds as the problem category. (2) Then, it prompts a generative language model with the sampled concepts to obtain both the problems and their step-wise formal solutions. (3) Lastly, the framework utilizes a proof assistant (e.g., Lean Prover) to filter the valid proofs. With the proposed MUSTARD, we present a theorem-and-proof benchmark MUSTARDSAUCE with 5,866 valid data points. Each data point contains an informal statement, an informal proof, and a translated formal proof that passes the prover validation. We perform extensive analysis and demonstrate that MUSTARD generates validated high-quality step-by-step data. We further apply the MUSTARDSAUCE for fine-tuning smaller language models. The fine-tuned Llama 2-7B achieves a 15.41% average relative performance gain in automated theorem proving, and 8.18% in math word problems. Codes and data are available at https://github.com/Eleanor-H/MUSTARD.
Buccinum strigilatum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Buccinidae
Buccinum
Buccinum strigilatum

description: Buccinum strigilatum [spec. nov.]
B. testa turrita oblique striata.
Rumph. mus. t. 30. f. H.
Gvalt. test. t. 57. f. O.
Argenv. conch. t. 14. f. R.
Habitat in O. Asiatico.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 741-742, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Potier et al. data and quantum catch table from High resolution of colour vision, but low contrast sensitivity in a diurnal raptor
Creators: name: POTIER, Simon
name: Mitkus, Mindaugas
name: Kelber, Almut
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Neuroscience
subject: 60801 Animal Behaviour
subject: FOS: Biological sciences

description: Animals are thought to use achromatic signals to detect small (or distant) objects and chromatic signals for large (or nearby) objects. While the spatial resolution of the achromatic channel has been widely studied, the spatial resolution of the chromatic channel has rarely been estimated. Using an operant conditioning method, we determined (i) the achromatic contrast sensitivity function and (ii) the spatial resolution of the chromatic channel of a diurnal raptor, the Harris's hawk Parabuteo unicinctus. The maximal spatial resolution for achromatic gratings was 62.3 c deg−1, but the contrast sensitivity was relatively low (10.8–12.7). The spatial resolution for isoluminant red-green gratings was 21.6 c deg−1—lower than that of the achromatic channel, but the highest found in the animal kingdom to date. Our study reveals that Harris's hawks have high spatial resolving power for both achromatic and chromatic vision, suggesting the importance of colour vision for foraging. By contrast, similar to other bird species, Harris's hawks have low contrast sensitivity possibly suggesting a trade-off with chromatic sensitivity. The result is interesting in the light of the recent finding that double cones—thought to mediate high-resolution vision in birds—are absent in the central fovea of raptors.
Cosmological Constant and Soft Terms in Supergravity
Creators: name: Choi, Kiwoon
name: Kim, Jihn E.
name: Nilles, Hans Peter
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Some of the soft SUSY breaking parameters in hidden sector supergravity model depend on the expectation value of the hidden sector scalar potential, $$, whose tree level value is equal to the tree level cosmological constant. The current practice of calculating soft parameters assumes that $=0$. Quantum correction to the cosmological constant can differ from the correction to $$ by an amount of order $m^2_{3/2}M_{Pl}^2/8π$. This implies that, for the vanishing cosmological constant, the $$--dependent parts of soft terms can be sizable, and hence the supergravity phenomenology should be accordingly modified.
description: Latex file, 11 pages plus 1 figure (the figure not included), SNUTP 94--19
Radiation mediated shocks in gamma-ray bursts: Subshock photon production
Creators: name: Lundman, Christoffer
name: Beloborodov, Andrei
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Internal shocks provide a plausible heating mechanism in the jets of gamma-ray bursts (GRBs). Shocks occurring below the jet photosphere are mediated by radiation. It was previously found that radiation mediated shocks (RMSs) inside GRB jets are inefficient photon producers, and the photons that mediate the RMS must originate from an earlier stage of the explosion. We show that this conclusion is valid only for non-magnetized jets. RMSs that propagate in moderately magnetized plasma develop a collisionless subshock which locally heats the plasma to a relativistic temperature, and the hot electrons emit copious synchrotron photons inside the RMS. We find that this mechanism is generally effective for mildly relativistic shocks and may be the main source of photons observed in GRBs. We derive a simple analytical formula for the generated photon number per proton, $Z$, which gives $Z=10^5$-$10^6$, consistent with observations. The photons are initially injected with low energies, well below the observed GRB peak. Their number is controlled by two main factors: (1) the abundance of electron-positron pairs created in the shock, which is self-consistently calculated, and (2) the upper limit on the brightness temperature of soft radiation set by induced downscattering. The injected soft photons that survive induced downscattering gain energy in the RMS via bulk Comptonization and shape its nonthermal spectrum.
description: 10 pages, submitted to ApJ
Cosmic radioactivities
Creators: name: Arnould, Marcel
name: Prantzos, Nikos
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Radionuclides with half-lives ranging from some years to billions of years presumably synthesized outside of the solar system are now recorded in ``live'' or ``fossil'' form in various types of materials, like meteorites or the galactic cosmic rays. They bring specific astrophysical messages the deciphering of which is briefly reviewed here, with special emphasis on the contribution of Dave Schramm and his collaborators to this exciting field of research. Short-lived radionuclides are also present in the Universe today, as directly testified by the gamma-ray lines emitted by the de-excitation of their daughter products. A short review of recent developments in this field is also presented.
description: Invited Review to appear in New Astronomy, 16 pages, 2 figures
Additional file 15 of GhCIPK6a increases salt tolerance in transgenic upland cotton by involving in ROS scavenging and MAPK signaling pathways
Creators: name: Su, Ying
name: Guo, Anhui
name: Huang, Yi
name: Wang, Yumei
name: Hua, Jinping
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 15: Figure S10. Analysis of differences in amino acid sequences and phosphorylation sites between GhCIPK6a (HM002633) and GhCIPK6 (KC465063). A. Sequence alignment of GhCIPK6a (HM002633) and GhCIPK6 (KC465063). B. Schematic of predicted phosphorylation sites of GhCIPK6s by KinasePhos ( http://kinasephos.mbc.nctu.edu.tw/ ).
Spectral variations within solar flare ribbons
Creators: name: Pietrow, A. G. M.
name: Druett, M. K.
name: Singh, V.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Solar flare ribbons are intense brightenings of principally chromospheric material that are responsible for a large fraction of the chromospheric emission in solar and stellar flares. We present an on-disc observation of flare ribbon substructures in an X9.3-class flare observed by the Swedish 1-m Solar Telescope. We identify categories of ribbon substructures seen in the Ca II 8542 Å, H$α$, and Ca II K lines, focusing on their spatial locations and their (spectro-)polarimetric properties. Color Collapsed Plotting (COCOPLOT) software is used to assist in identifying areas of interest. We present five categories of spectral profiles within the general body of the flare ribbon: (1) Extremely broadened spectral line profiles, where the standard Fabry-Perot interferometer wavelength windows ($\approx 70$ km s$^{-1}$) are insufficiently wide to allow for a complete analysis of the dynamics and atmospheric conditions. The mechanisms causing this degree of this broadening are not yet clearly understood. (2) Long-lived, dense kernels that manifest as more saturated chromospheric line profiles with lower signal in both Stokes parameters. They are interpreted as footpoints of bunched magnetic field loops, whose chromospheric lines form at greater heights than the nearby areas. (3) Doppler-shifted leading edges of the flare ribbon in regions that transiently display lower Stokes signals due to the emission dominating at greater heights in the atmosphere. (4) Condensed coronal rain overlapping the flare ribbons in the line of sight, producing exceptionally high Doppler shifts near the footpoints...
description: Published in A&A. 11 pages, 8 figures
Buccinum duplicatum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Buccinidae
Buccinum
Buccinum duplicatum

description: Buccinum duplicatum [spec. nov.]
B. testa turrita, anfractibus bipartitis striatis.
Gvalt. test. t. 57. f. N.
Habitat in O. Indico.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 742, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Buccinum dimidiatum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Buccinidae
Buccinum
Buccinum dimidiatum

description: Buccinum dimidiatum [spec. nov.]
B. testa turrita, anfractibus bifidis laevibus.
Habitat in O. Africano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 742, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quantum phases of a three-level matter-radiation interaction model using $SU(3)$ coherent states with different cooperation numbers
Creators: name: Quezada, L. F.
name: Nahmad-Achar, E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We use coherent states as trial states for a variational approach to study a system of a finite number of three-level atoms interacting in a dipolar approximation with a one-mode electromagnetic field. The atoms are treated as semi-distinguishable using different cooperation numbers and representations of SU(3). We focus our analysis on the quantum phases of the system as well as the behavior of the most relevant observables near the phase transitions. The results are computed for all three possible configurations ($Ξ$, $Λ$ and $V$) of the three-level atoms.
description: 9 pages, 13 figures. arXiv admin note: text overlap with arXiv:1712.01889
Additional file 1 of The Incidence of Sports-Related Concussion in Children and Adolescents: A Systematic Review and Meta-Analysis
Creators: name: Ingram, Veronica
name: Fielding, Megan
name: Dunne, Laura A. M.
name: Piantella, Stefan
name: Weakley, Jonathon
name: Johnston, Rich D.
name: McGuckian, Thomas B.
Publisher: name: figshare
Year: 2025
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Cancer
Science Policy

description: Supplementary file 1
Exact Multiparticle Amplitudes at Threshold in Large-N Component phi^4 Theory
Creators: name: Makeenko, Yu.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: I derive the set of recurrence relations between the amplitudes of multiparticle production at threshold in the standard large-N limit of the O(N)-symmetric phi^4$ theory which sums all relevant diagrams with arbitrary number of loops. I find an exact solution to the recurrence relations using the Gelfand--Dikii representation of the diagonal resolvent of the Schrodinger operator. The result coincides with the tree amplitudes while the effect of loops is the renormalization of the coupling constant and mass. The form of the solution is due to the fact that the exact amplitude of the process 2->n at n>2 vanishes on mass shell when averaged over the O(N)-indices of incoming particles for dynamical reasons because of the cancellation between diagrams. I discuss some possible applications of large-N amplitudes, in particular, for the renormalon problem.
description: 18 pp., Latex (6 Latex figures), NBI-HE-94-25
Revealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety
Creators: name: Gendron-Marsolais, M.
name: Hlavacek-Larrondo, J.
name: Martin, T. B.
name: Drissen, L.
name: McDonald, M.
name: Fabian, A. C.
name: Edge, A. C.
name: Hamer, S. L.
name: McNamara, B.
name: Morrison, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have produced for the first time a detailed velocity map of the giant filamentary nebula surrounding NGC 1275, the Perseus cluster's brightest galaxy, and revealed a previously unknown rich velocity structure across the entire nebula. We present new observations of the low-velocity component of this nebula with the optical imaging Fourier transform spectrometer SITELLE at CFHT. With its wide field of view ($\sim$11'$\times$11'), SITELLE is the only integral field unit spectroscopy instrument able to cover the 80 kpc$\times$55 kpc (3.8'$\times$2.6') large nebula in NGC 1275. Our analysis of these observations shows a smooth radial gradient of the [N II]$λ$6583/$\text{H} α$ line ratio, suggesting a change in the ionization mechanism and source across the nebula, while the dispersion profile shows a general decrease with increasing distance from the AGN at up to $\sim 10$ kpc. The velocity map shows no visible general trend or rotation, indicating that filaments are not falling uniformly onto the galaxy, nor being pulled out from it. Comparison between the physical properties of the filaments and Hitomi measurements of the X-ray gas dynamics in Perseus are also explored.
description: 5 pages, 6 figures, submitted to MNRAS Letters
C^+ distribution around S1 in rho Ophiuchi
Creators: name: Mookerjea, B.
name: Sandell, G.
name: Vacca, W.
name: Chambers, E.
name: Guesten, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We analyze a [C II] 158 micron map obtained with the L2 GREAT receiver on SOFIA of the emission/reflection nebula illuminated by the early B star S1 in the rho-OphA cloud core. This data set has been complemented with maps of CO(3-2), 13CO(3-2) and C18O(3-2), observed as a part of the JCMT Gould Belt Survey, with archival HCO^+(4-3) JCMT data, as well as with [O I] 63 and 145 micron imaging with Herschel/PACS. The [C II] emission is completely dominated by the strong PDR emission from the nebula surrounding S1 expanding into the dense Oph A molecular cloud west and south of S1. The [C II] emission is significantly blue shifted relative to the CO spectra and also relative to the systemic velocity, particularly in the northwestern part of the nebula. The [C II] lines are broader towards the center of the S1 nebula and narrower towards the PDR shell. The [C II] lines are strongly self-absorbed over an extended region in the S1 PDR. Based on the strength of the [13C II] F = 2-1 hyperfine component, [C II] is significantly optically thick over most of the nebula. CO and 13CO(3-2) spectra are strongly self-absorbed, while C18O(3-2) is single peaked and centered in the middle of the self-absorption. We have used a simple two-layer LTE model to characterize the background and foreground cloud contributing to the [C II] emission. From this analysis we estimate the extinction due to the foreground cloud to be ~9.9 mag, which is slightly less than the reddening estimated towards S1. Since some of the hot gas in the PDR is not traced by low J CO emission, this result appears quite plausible. Using a plane parallel PDR model with the observed [OI(145)]/[C II] brightness ratio and an estimated FUV intensity of 3100-5000 G0 suggests that the density of the [C II] emitting gas is ~3-4x10^3 cm^-3.
description: Accepted for publication in Astronomy & Astrophysics
Additional file 1 of Validation of a microRNA profile in urine liquid biopsy with diagnostic and stratification value for bladder cancer classification, available through the open app BladdermiRaCan
Creators: name: Oto, Julia
name: Herranz, Raquel
name: Plana, Emma
name: Pérez-Ardavín, Javier
name: Hervás, David
name: Cana, Fernando
name: Verger, Patricia
name: Ramos-Soler, David
name: Martínez-Sarmiento, Manuel
name: Vera-Donoso, César D.
name: Medina, Pilar
Publisher: name: figshare
Year: 2025
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Astronomical and Space Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Supplementary Material 1
title: ADCO, Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Cart. 184 (11 H 987), 105 folios, f. 0182
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0182, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0182, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
All electroweak four fermion processes in electron-positron collisions
Creators: name: Berends, F. A.
name: Kleiss, R.
name: Pittau, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: This paper studies the electroweak production of all possible four fermion states in e+ e- collisions. Since the methods employed to evaluate the complete matrix elements and phase space are very general, all four fermion final states in which the charged particles are detected can be considered. Also all kinds of experimental cuts can be imposed. With the help of the constructed event generator a large number of illustrative results is obtained, which show the relevance of backgrounds to a number of signals. For LEP 200 the W-pair signal and its background are discussed, for higher energies also Z-pair and single W and Z signals and backgrounds are presented.
description: INLO-PUB-1/94,NIKHEF-H/94-08, LaTeX, uses axodraw.sty (appended to end of TeX file), 45 pages
KURASH SPORT MUSOBAQALARIGA TAYYORLASHDA  JISMONIY SIFATLARNING AHAMIYATI
Creators: name: Ikramov, Ilxom
name: Ro'ziboyeva, Nigina
Publisher: name: Zenodo
Year: 2024

description: Ushbu maqolada  Kurash sport turining xalqona xususiyatlari va uning milliy ruhi, obro‘si haqida fikr yuritiladi.
Stability of a dispersion of elongated particles embedded in a viscous membrane
Creators: name: Manikantan, Harishankar
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We develop a mean-field model to examine the stability of a `quasi-2D suspension' of elongated particles embedded within a viscous membrane. This geometry represents several biological and synthetic settings, and we reveal mechanisms by which the anisotropic mobility of particles interacts with long-ranged viscous membrane hydrodynamics. We first show that a system of slender rod-like particles driven by a constant force is unstable to perturbations in concentration -- much like sedimentation in analogous 3D suspensions -- so long as membrane viscous stresses dominate. However, increasing the contribution of viscous stresses from the surrounding 3D fluid(s) suppresses such an instability. We then tie this result to the hydrodynamic disturbances generated by each particle in the plane of the membrane and show that enhancing subphase viscous contributions generates extensional fields that orient neighboring particles in a manner that draws them apart. The balance of flux of particles aggregating versus separating then leads to a wave number selection in the mean-field model.
Buccinum murinu Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Buccinidae
Buccinum
Buccinum murinu

description: Buccinum murinu [spec. nov.]
B. testa turrita, anfractibus subangulatis, striis tribus muricatis.
Gvalt. test. t. 57. f. P.
Habitat ad Africam.
Testa nigra basi gibba, anfractibus saepe basi albis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 742, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Efficient, mild synthesis of N-unsubstituted 1,2,3-triazoles from methanolysis of 1-sulfonyl-1,2,3-triazoles
Creators: name: Rodríguez-Florencio, Janeth
name: Martínez-Otero, Diego
name: García-Eleno, Marco A.
name: Cuevas-Yañez, Erick
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: A small library of diverse N-unsubstituted 1,2,3-triazoles was prepared from the corresponding 1-sulfonyl-1,2,3-triazoles, which were treated only with MeOH at reflux temperature. This process was carried out in good yields showing high efficiency and good functional group tolerance.
Detection of hard X-rays from a Class I protostar in the HH24-26 region in the Orion Molecular Cloud
Creators: name: Ozawa, H.
name: Nagase, F.
name: Ueda, Y.
name: Dotani, T.
name: Ishida, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We observed the HH24-26 region in the L1630 Orion molecular cloud complex with the X-ray observatory ASCA in the 0.5$-$10 keV band. X-ray emission was detected from the T Tauri star SSV61 and from the region where the Class I protostars SSV63E and SSV63W are located (hereafter SSV63E+W). The spectra of both SSV63E+W and SSV61 are well explained by an optically thin thermal plasma model. The spectrum of the T Tauri star SSV61 has a low temperature of $kT=0.9$ (0.7$-$1.2) keV and a moderate absorption of $N_{\rm{H}}=1.3$ (0.9$-$1.7) $\times10^{22}$ cm$^{-2}$, while that of the protostar SSV63E+W has a high temperature of $kT=5.0$ (3.3$-$7.9) keV and a heavy absorption of $N_{\rm{H}}=1.5$ (1.2$-$1.8) $\times10^{23}$ cm$^{-2}$. The X-ray light curve of SSV63E+W showed a flare during the observation. The peak flux reached about 9 times that of the quiescent flux. The temperature and the absorption column density do not change conspicuously during the flare. The 0.5$-$10 keV luminosity of SSV63E+W was about $1\times10^{32}$ erg s$^{-1}$ in the quiescent state. The present detection of hard X-rays from SSV63E+W is remarkable, because this is the first X-ray detection of a protostar in Orion.
description: 14 pages, 3 postscript figures, uses aasms4.sty
Neutral Gas Distribution and Kinematics of the Nearly Face-on Spiral Galaxy NGC 1232
Creators: name: van Zee, L.
name: Bryant, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have analyzed high velocity resolution HI synthesis observations of the nearly face-on Sc galaxy NGC 1232. The neutral gas distribution extends well beyond the optical extent of the galaxy. As expected, local peaks in the HI column density are associated with the spiral arms. Further, the HI column density drops precipitously near the center of the galaxy. Closed contours in the velocity field suggest either that the system is warped, or that the rotation curve declines. The velocity dispersion is approximately constant throughout the system, with a median value of 9.9 +/- 1.8 km/s. When corrected for rotational broadening, there is no indication of a radial trend in the neutral gas velocity dispersion in this galaxy.
description: 14 pages of text, 10 pages of figures. Accepted to the AJ
Rossby Wave Instability of Thin Accretion Disks -- II. Detailed Linear Theory
Creators: name: Li, H.
name: Finn, J. M.
name: Lovelace, R. V. E.
name: Colgate, S. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In earlier work we identified a global, non-axisymmetric instability associated with the presence of an extreme in the radial profile of the key function ${\cal L}(r) \equiv (ΣΩ/κ^2) S^{2/Γ}$ in a thin, inviscid, nonmagnetized accretion disk. Here, $Σ(r)$ is the surface mass density of the disk, $Ω(r)$ the angular rotation rate, $S(r)$ the specific entropy, $Γ$ the adiabatic index, and $κ(r)$ the radial epicyclic frequency. The dispersion relation of the instability was shown to be similar to that of Rossby waves in planetary atmospheres. In this paper, we present the detailed linear theory of this Rossby wave instability and show that it exists for a wider range of conditions, specifically, for the case where there is a ``jump'' over some range of $r$ in $Σ(r)$ or in the pressure $P(r)$. We elucidate the physical mechanism of this instability and its dependence on various parameters, including the magnitude of the ``bump'' or ``jump,'' the azimuthal mode number, and the sound speed in the disk. We find large parameter range where the disk is stable to axisymmetric perturbations, but unstable to the non-axisymmetric Rossby waves. We find that growth rates of the Rossby wave instability can be high, $\sim 0.2 Ω_{\rm K}$ for relative small ``jumps'' or ``bumps''. We discuss possible conditions which can lead to this instability and the consequences of the instability.
description: Use emulapj style, 14 pages, 12 figures, submitted to ApJ
Additional file 4 of Large-scale public data reuse to model immunotherapy response and resistance
Creators: name: Fu, Jingxin
name: Li, Karen
name: Zhang, Wubing
name: Wan, Changxin
name: Zhang, Jing
name: Jiang, Peng
name: Liu, X.
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences

description: Figure S1. The prediction performance of recently published biomarkers varies across data cohorts; and Supplementary Methods.
title: Characterization of Prokaryotic and Eukaryotic Biodiversity from Soil Samples
Creators: name: Chaves, Cátia
name: Najera Cortazar, Laura
name: Martins, Filipa
name: Anslan, Sten
name: Beja-Pereira, Albano
name: Magalhães, Maria
name: Price, Ben
Publisher: name: WorkflowHub
Year: 2025

description: SOP for DNA extraction and Illumina amplicon library preparation of soil core samples collected for the Case Study "Characterization of Prokaryotic and Eukaryotic Biodiversity from Soil Samples" withing the scope of BGE (Biodiversity Genomics Europe) project.
X States of the Same Spectrum and Entanglement as All Two-Qubit States
Creators: name: Hedemann, Samuel R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present an explicit family of two-qubit X states with entanglement-preserving unitary (EPU) equivalence to the set of general states; that is, for any spectrum-entanglement combination achievable by general states, this family contains an X state of the same spectrum and entanglement. This idea was originally conjectured by the author and supported with strong numerical evidence in arXiv:1310.7038. Then, in Ann. Phys. 351 (2014) 79, the authors proved the existence of such two-qubit unitary transformations, but found the parameters to be transcendental, eluding explicit solution. Here, by a different method, we prove the existence of such transformations, obtain a compact implicit solution for them, and provide an exact, explicit form of the desired X-state family.
description: 7 pages, 3 figures
HST Observations of the Serendipitous X-ray Companion to Mrk 273: Cluster at z=0.46?
Creators: name: Borne, K. D.
name: Colina, L.
name: Bushouse, H.
name: Lucas, R. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used HST I-band images to identify Mrk 273X, the very unusual high-redshift X-ray-luminous Seyfert 2 galaxy found by ROSAT in the same field-of-view as Mrk 273. We have measured the photometric properties of Mrk 273X and have also analyzed the luminosity distribution of the faint galaxy population seen in the HST image. The luminosity of the galaxy and the properties of the surrounding environment suggest that Mrk 273X is the brightest galaxy in a relatively poor cluster at a redshift near 0.46. Its off-center location in the cluster and the presence of other galaxy groupings in the HST image may indicate that this is a dynamically young cluster on the verge of merging with its neighboring clusters. We find that Mrk 273X is a bright featureless elliptical galaxy with no evidence for a disk. It follows the de Vaucouleurs (r^{1/4}) surface brightness law very well over a range of 8 magnitudes. Though the surface brightness profile does not appear to be dominated by the AGN, the galaxy has very blue colors that do appear to be produced by the AGN. Mrk 273X is most similar to the IC 5063 class of active galaxies --- a hybrid Sy 2 / powerful radio galaxy.
description: Accepted for publication in the Astrophysical Journal. 8 pages, including 4 postscript figures. Uses emulateapj.sty and psfig.sty. Higher quality version of Figure 1 is available at http://rings.gsfc.nasa.gov/~borne/fig1-markgals.gif
Chiral Invariance of Massive Fermions
Creators: name: Das, A.
name: Hott, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that a massive fermion theory, while not invariant under the conventional chiral transformation, is invariant under a $m$-deformed chiral transformation. These transformations and the associated conserved charges are nonlocal but reduce to the usual transformations and charges when $m=0$. The $m$-deformed charges commute with helicity and satisfy the conventional chiral algebra.
description: 12 pages, UR-1352, ER-40685-803
The Linear Polarization of Sagittarius A* II. VLA and BIMA Polarimetry at 22, 43 and 86 GHz
Creators: name: Bower, Geoffrey C.
name: Wright, Melvyn C. H.
name: Backer, Donald C.
name: Falcke, Heino
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a search for linear polarization at 22 GHz, 43 GHz and 86 GHz from the nearest super massive black hole candidate, Sagittarius A*. We find upper limits to the linear polarization of 0.2%, 0.4% and 1%, respectively. These results strongly support the conclusion of our centimeter wavelength spectro-polarimetry that Sgr A* is not depolarized by the interstellar medium but is in fact intrinsically depolarized.
description: Accepted for publication in ApJ, 13 pages, 2 figures
Strombus pes pelecani Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Littorinimorpha
Strombidae
Strombus
Strombus pes pelecani

description: Strombus pes pelecani [spec. nov.]
S. testae la{?X}bro tetradactylo palmato digitis angulato, fauce laevi.
Bonan. recr. 3. t. 85, 87.
List. conch. t. 866. f. min.
Gvalt. test t. 53. f. B. C.
Argenv. conch. t. 17. f. M.
Habitat in O. Europaeo, Norvegico, Mediterraneo, Americano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 742, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Is \lq\lq Heavy Quark Damping Rate Puzzle'' in Hot QCD Really the Puzzle?
Creators: name: Niégawa, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Within the framework of perturbative resummation scheme of Pisarski and Braaten, the decay- or damping-rate of a moving heavy quark (muon) to leading order in weak coupling in hot QCD (QED) is examined. Although, as is well known, the conventionally-defined damping rate diverges logarithmically at the infrared limit, shown is that no such divergence appears in the physically measurable decay rate. The cancellation occurs between the contribution from the \lq\lq real'' decay diagram and the contribution from the diagrams with \lq\lq thermal radiative correction''.
description: 13pages, OCU-PHYS-154
Geographies of youth leadership: volunteering and the Young Leaders scheme in the UK Scout Association
Creators: name: Austin, Rosemary
Publisher: name: Loughborough University
Year: 2020
Subjects: subject: 49999 Earth Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences

description: Geographies of youth leadership: volunteering and the Young Leaders scheme in the UK Scout Association
Utilizing U-Net Architectures with Auxiliary Information for Scatter Correction in CBCT Across Different Field-of-View Settings
Creators: name: Agrawal, Harshit
name: Hietanen, Ari
name: Särkkä, Simo
Publisher: name: arXiv
Year: 2024
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Cone-beam computed tomography (CBCT) has become a vital imaging technique in various medical fields but scatter artifacts are a major limitation in CBCT scanning. This challenge is exacerbated by the use of large flat panel 2D detectors. The scatter-to-primary ratio increases significantly with the increase in the size of FOV being scanned. Several deep learning methods, particularly U-Net architectures, have shown promising capabilities in estimating the scatter directly from the CBCT projections. However, the influence of varying FOV sizes on these deep learning models remains unexplored. Having a single neural network for the scatter estimation of varying FOV projections can be of significant importance towards real clinical applications. This study aims to train and evaluate the performance of a U-Net network on a simulated dataset with varying FOV sizes. We further propose a new method (Aux-Net) by providing auxiliary information, such as FOV size, to the U-Net encoder. We validate our method on 30 different FOV sizes and compare it with the U-Net. Our study demonstrates that providing auxiliary information to the network enhances the generalization capability of the U-Net. Our findings suggest that this novel approach outperforms the baseline U-Net, offering a significant step towards practical application in real clinical settings where CBCT systems are employed to scan a wide range of FOVs.
Additional file 1 of Inflammatory and lipemic response to red meat intake in women with and without Rheumatoid Arthritis: a single meal study within a randomized controlled trial
Creators: name: Sällström, Torsten
name: Bärebring, Linnea
name: Hulander, Erik
name: Gjertsson, Inger
name: Winkvist, Anna
name: Lindqvist, Helen M.
Publisher: name: figshare
Year: 2025
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified

description: Additional file 1