cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Cluster-EAGLE project: a comparison of dynamical mass estimators using simulated clusters
Creators: name: Armitage, Thomas J.
name: Kay, Scott T.
name: Barnes, David J.
name: Bahé, Yannick M.
name: Vecchia, Claudio Dalla
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Forthcoming large-scale spectroscopic surveys will soon provide data on thousands of galaxy clusters. It is important that the systematics of the various mass estimation techniques are well understood and calibrated. We compare three different dynamical mass estimators using the C-EAGLE galaxy clusters, a set of high resolution simulations with resolved galaxies a median total mass, $M_{200c} = 10^{14.7} \, \mathrm{M_\odot}$. We quantify the bias and scatter of the Jeans, virial, and caustic mass estimators using all galaxies with a stellar mass $M_*> 10^9 \, \mathrm{M_\odot}$, both in the ideal 3D case and in the more realistic projected case. On average we find our mass estimates are unbiased, though relative to the true mass within $r_{200c}$ the scatter is large with a range of $0.09$ - $0.15$ dex. We see a slight increase in the scatter when projecting the clusters. Selecting galaxies using the same criteria, we find no significant difference in the mass bias or scatter when comparing results from hydrodynamical and dark matter only simulations. However, selecting galaxies by stellar mass reduces the bias compared to selecting by total mass. Comparing X-ray derived hydrostatic and dynamical masses, the former are ${\sim} 30$ per cent lower. We find a slight dependence between substructure, measured using two different metrics, and mass bias. In conclusion, we find that dynamical mass estimators, when averaged together, are unbiased with a scatter of $0.11 \pm 0.02$ dex when including interloper galaxies and with no prior knowledge of $r_{200c}$.
description: Accepted in MNRAS, 14 figures in main text
Asymptotics of Elliptic Genera of Symmetric Products and Dyonic Black Hole Degeneracy
Creators: name: Bytsenko, A. A.
name: Goncalves, A. E.
name: Odintsov, S. D.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We calculate asymptotic expansions of elliptic genera for a supersymmetric sigma model on the N - fold symmetric product S^NM of a Kahler manifold M and for N = 2 superconformal field theory. Asymptotic expansions for the degeneracy of dyonic black hole spectrum are also derived.
description: 11 pages, LaTeX, two news refs. have been added
The Norris Survey of the Corona Borealis Supercluster: II. Galaxy Evolution with Redshift and Environment
Creators: name: Small, Todd A.
name: Sargent, Wallace L. W.
name: Hamilton, Donald
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We measure the field galaxy luminosity function (LF) as a function of color and redshift from z = 0 to z = 0.5 using galaxies from the Norris Survey of the Corona Borealis Supercluster. We find that our local r-band LF, when normalized to counts in high galactic latitude fields, agrees well with the local LF measured in the Las Campanas Redshift Survey. Our B-band local LF, however, does not match the B-band LF from the Stromlo/APM survey, having a normalization 1.6 times higher. We see compelling evidence that B-band field galaxy LF evolves with redshift. The evolution is strongest for the population of star-forming galaxies with [OII]3727 rest-frame equivalent widths greater than 10A. The population of red, quiescent galaxies shows no sign of evolution to z = 0.5. The evolution of the LF which we observe is consistent with the findings of other faint galaxy redshift surveys. The fraction of galaxies with [OII] emission increases rapidly with redshift, but the fraction of galaxies with strong Hdelta 4101 absorption, a signature of a burst of star formation, does not. We thus conclude that the star formation in distant galaxies is primarily long-lived. We also compute the LFs of the Corona Borealis supercluster and the A2069 supercluster. The shapes of the two supercluster LFs are broadly similar to the shape of the local LF. However, there are important differences. Both supercluster LFs have an excess of very bright galaxies. In addition, there is a suggestion of an upturn in the LF for galaxies fainter than M(B) = -17 mag. (Abridged from the abstract in the paper.)
description: 28 pages plus 18 pages of figures; accepted for publication in ApJ
A Persistent Disk Wind in GRS 1915+105 with NICER
Creators: name: Neilsen, Joey
name: Cackett, E.
name: Remillard, R. A.
name: Homan, J.
name: Steiner, J. F.
name: Gendreau, K.
name: Arzoumanian, Z.
name: Prigozhin, G.
name: LaMarr, B.
name: Doty, J.
name: Eikenberry, S.
name: Tombesi, F.
name: Ludlam, R.
name: Kara, E.
name: Altamirano, D.
name: Fabian, A. C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The bright, erratic black hole X-ray binary GRS 1915+105 has long been a target for studies of disk instabilities, radio/infrared jets, and accretion disk winds, with implications that often apply to sources that do not exhibit its exotic X-ray variability. With the launch of NICER, we have a new opportunity to study the disk wind in GRS 1915+105 and its variability on short and long timescales. Here we present our analysis of 39 NICER observations of GRS 1915+105 collected during five months of the mission data validation and verification phase, focusing on Fe XXV and Fe XXVI absorption. We report the detection of strong Fe XXVI in 32 (>80%) of these observations, with another four marginal detections; Fe XXV is less common, but both likely arise in the well-known disk wind. We explore how the properties of this wind depends on broad characteristics of the X-ray lightcurve: mean count rate, hardness ratio, and fractional RMS variability. The trends with count rate and RMS are consistent with an average wind column density that is fairly steady between observations but varies rapidly with the source on timescales of seconds. The line dependence on spectral hardness echoes known behavior of disk winds in outbursts of Galactic black holes; these results clearly indicate that NICER is a powerful tool for studying black hole winds.
description: Accepted for publication in ApJL. Comments welcome
Impairment of α-tubulin and F-actin interactions of GJB3 induces aneuploidy in urothelial cells and promotes bladder cancer cell invasion
Creators: name: Liu, Junnan
name: Wang, Xue
name: Jiang, Wencheng
name: Azoitei, Anca
name: Eiseler, Tim
name: Eckstein, Markus
name: Hartmann, Arndt
name: Stilgenbauer, Stephan
name: Elati, Mohamed
name: Hohwieler, Meike
name: Kleger, Alexander
name: John, Axelinfo
name: Wezel, Felix
name: Zengerling, Friedemann H.
name: Bolenz, Christian
name: Günes̃, Çag̃atay
Publisher: name: Universität Ulm
Year: 2024
Subjects: subject: Spindle orientation
subject: Chromosomal imbalance
subject: Invadopodia
subject: Metastasis
subject: MIBC
subject: DDC 610 / Medicine & health

description: Background We have previously identified an unsuspected role for GJB3 showing that the deficiency of this connexin protein induces aneuploidy in human and murine cells and accelerates cell transformation as well as tumor formation in xenograft models. The molecular mechanisms by which loss of GJB3 leads to aneuploidy and cancer initiation and progression remain unsolved. Methods GJB3 expression levels were determined by RT-qPCR and Western blot. The consequences of GJB3 knockdown on genome instability were assessed by metaphase chromosome counting, multinucleation of cells, by micronuclei formation and by the determination of spindle orientation. Interactions of GJB3 with α-tubulin and F-actin was analyzed by immunoprecipitation and immunocytochemistry. Consequences of GJB3 deficiency on microtubule and actin dynamics were measured by live cell imaging and fluorescence recovery after photobleaching experiments, respectively. Immunohistochemistry was used to determine GJB3 levels on human and murine bladder cancer tissue sections. Bladder cancer in mice was chemically induced by BBN-treatment. Results We find that GJB3 is highly expressed in the ureter and bladder epithelium, but it is downregulated in invasive bladder cancer cell lines and during tumor progression in both human and mouse bladder cancer. Downregulation of GJB3 expression leads to aneuploidy and genomic instability in karyotypically stable urothelial cells and experimental modulation of GJB3 levels alters the migration and invasive capacity of bladder cancer cell lines. Importantly, GJB3 interacts both with α-tubulin and F-actin. The impairment of these interactions alters the dynamics of these cytoskeletal components and leads to defective spindle orientation. Conclusion We conclude that deregulated microtubule and actin dynamics have an impact on proper chromosome separation and tumor cell invasion and migration. Consequently, these observations indicate a possible role for GJB3 in the onset and spreading of bladder cancer and demonstrate a molecular link between enhanced aneuploidy and invasive capacity cancer cells during tumor cell dissemination.
What's new at small x
Creators: name: Venugopalan, Raju
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We discuss some recent developments in small x physics.
description: LaTex, 12 pages .Plenary talk at WHEPP-6, Chennai, India, Jan.3rd-15th, 2000
MOESM1 of Proteinase K treatment improves RNA recovery from thyroid cells fixed with liquid-based cytology solution
Creators: name: Jikuzono, Tomoo
name: Horikawa, Aya
name: Ishikawa, Tomoko
name: Hirokawa, Mitsuyoshi
name: Sugitani, Iwao
name: Inui, Takashi
name: Ishibashi, Osamu
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: Additional file 1: Figure S1. Cell trapping in a glass-fiber filter. (A) Scheme of cell trapping in a glass-fiber filter and RNA isolation. Cell suspension in a fixative was passed through the glass-fiber filter to trap the cells. The filter with trapped cells was subjected to RNA isolation. (B) Verification of cell trapping. Microscopic images of the cell suspension before and after filtration. After the K1 cell suspension was passed through the glass-fiber filter, only few cells were observed in the filtrate, indicating that the cells were efficiently trapped in the grass-fiber filter. Figure S2. Detection of RNU6 RNA in RNA samples isolated from materials fixed with LBC solution. The total RNA (10Â ng per reaction) isolated from the CytoRich-fixed K1 cells and thyroid FNAB specimens that were treated with Proteinase K was subjected to TaqMan-based quantitative RT-PCR to detect RNU6 RNA. Assays were performed in triplicates. No amplification was observed when a cDNA template was omitted from the reaction (negative control).
1928 Excavations at Casa Grande Ruins
Creators: name: Gladwin, Harold S.
Publisher: name: Southwest Musuem
Year: 1928
Subjects: subject: Middle Gila River Basin
valueUri: https://core.tdar.org/browse/geographic-keyword/54303/middle-gila-river-basin
subject: Classic Period
valueUri: https://core.tdar.org/browse/temporal-keyword/125/classic-period
subject: Sedentary Period
valueUri: https://core.tdar.org/browse/temporal-keyword/5504/sedentary-period
subject: Colonial Period
valueUri: https://core.tdar.org/browse/temporal-keyword/5377/colonial-period
subject: Hohokam
valueUri: https://core.tdar.org/browse/culture-keyword/21/hohokam
subject: Casa Grande Ruins, Adamsville, the Grewe site
valueUri: https://core.tdar.org/browse/site-name/1392/casa-grande-ruins-adamsville-the-grewe-site
subject: Archaeological Feature
valueUri: https://core.tdar.org/browse/site-type/339/archaeological-feature
subject: Non-Domestic Structures
valueUri: https://core.tdar.org/browse/site-type/309/non-domestic-structures
subject: Domestic Structure or Architectural Complex
valueUri: https://core.tdar.org/browse/site-type/251/domestic-structure-or-architectural-complex
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
subject: Ceramics & Chronology
valueUri: https://core.tdar.org/browse/other-keyword/107943/ceramics-chronology
subject: Archaeological Overview
valueUri: https://core.tdar.org/browse/investigation-type/1/archaeological-overview
subject: Historic Background Research
valueUri: https://core.tdar.org/browse/investigation-type/18/historic-background-research
subject: Data Recovery / Excavation
valueUri: https://core.tdar.org/browse/investigation-type/5/data-recovery-excavation
subject: Methodology, Theory, or Synthesis
valueUri: https://core.tdar.org/browse/investigation-type/6/methodology-theory-or-synthesis

description: Harold Gladwin's 1928 Excavations at Grande Ruins includes Gladwins investigations in 1927 at Casa Grande Ruins, the Grewe site, and Adamsville. While still at the Southwest Museum in Los Angeles, Gladwin conducted excavations at sites along the middle Gila River in an effort to create a ceramic typology for the area.
Cremastogaster platygnatha Roger
Creators: name: André, E.
Publisher: name: Zenodo
Year: 1890
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Cremastogaster
Cremastogaster platygnatha

description: Cremastogaster platygnatha Roger
(Formica platygnatha Hog., Berl. Ent. Zeit., 1863, p. 168. = Cr. mandibularis Andre, Revue d'Ent., 1889, p. 229)
Malgre le soin que j'apporte a ne publier aucune espece nouvelle sans m'etre assure, par l'etude attentive des descriptions anterieures, qu'elle n'a pas ele connue de mes devanciers, j'ai decrit dans cette Revue, sous le nom de Crem. mandibularis, une femelle remarquable parla conformation singuliere de ses mandibules, mais qui n'est autre que la Formica platygnatha Rog. C'est en lisant, par hasard, la description de Roger, que j'ai reconnu l'identite des deux especes; car - et c'est la mon excuse - personne n'eut ete chercher cet insecte dans le genre Formica ou Roger l'a place. La description de l'auteur berlinois avait ete faite d'apres un exemplaire prive de petiole et d'abdomen, et cette circonstance n'avait pas permis a cet excellent myrmecologiste d'assigner a son insecte sa veritable place dans la serie des genres et meme des grandes divisions de la famille. Je m' empresse donc de restituer a Roger la paternite de cette fourmi, en me contentant de la satisfaction d'avoir enrichi le genre Cremastogaster d'un de ses plus curieux representants.
description: Published as part of André, E., 1890, Matériaux pour servir a la faune myrmécologique de Sierra-Leone (Afrique occidentale)., pp. 311-327 in Revista de Entomologia 9 on page 323
Constraints on off-shell Higgs boson production and the Higgs boson total width in $ZZ\to4\ell$ and $ZZ\to2\ell2ν$ final states with the ATLAS detector
Creators: name: ATLAS Collaboration
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A measurement of off-shell Higgs boson production in the $ZZ\to4\ell$ and $ZZ\to2\ell2ν$ decay channels, where $\ell$ stands for either an electron or a muon, is performed using data from proton-proton collisions at a centre-of-mass energy of $\sqrt{s}=13$ TeV. The data were collected by the ATLAS experiment in 2015 and 2016 at the Large Hadron Collider, and they correspond to an integrated luminosity of 36.1 fb$^{-1}$. An observed (expected) upper limit on the off-shell Higgs signal strength, defined as the event yield normalised to the Standard Model prediction, of 3.8 (3.4) is obtained at 95% confidence level (CL). Assuming the ratio of the Higgs boson couplings to the Standard Model predictions is independent of the momentum transfer of the Higgs production mechanism considered in the analysis, a combination with the on-shell signal-strength measurements yields an observed (expected) 95% CL upper limit on the Higgs boson total width of 14.4 (15.2) MeV.
description: 38 pages in total, author list starting page 22, 3 figures, 3 tables, submitted to Phys. Lett. B. All figures including auxiliary figures are available at https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/HIGG-2017-06/
Charmonium Decay Physics
Creators: name: Gu, Y. F.
name: Tuan, S. F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recent experimental results on the decays of charmonium, together with related physics issues, are reviewed. Some future prospects are described.
description: 8 pages, latex, no figures. Invited talk at the 8th International Conference on Hadron Spectroscopy (Hadron99), Beijing, 24-28 august, 1999; to appear in Proceedings
Resonant thermoelectric transport in atomic chains with Fano defects
Creators: name: González, J. Eduardo
name: Sánchez, Vicenta
name: Wang, Chumin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Atomic clusters attached to a low-dimensional system, called Fano defects, produce rich wave interferences. In this work, we analytically found an enhanced thermoelectric figure-of-merit (ZT) in periodic atomic chains with Fano defects, compared to those without such defects. We further study self-assembled DNA-like systems with periodic and quasiperiodically placed Fano defects by using a real-space renormalization method developed for the Kubo-Greenwood formula, in which tight-binding and Born models are respectively used for the electric and lattice thermal conductivities. The results reveal that the quasiperiodicity could be another ZT-improving factor, whose long-range disorder inhibits low-frequency acoustic phonons insensitive to local defects.
description: Accepted version in MRS Communications
Osp(1,2)-covariant Lagrangian quantization of reducible massive gauge theories
Creators: name: Geyer, B.
name: Lavrov, P. M.
name: M"ulsch, D.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The osp(1,2)-covariant Lagrangian quantization of irreducible gauge theories [hep-th/9712204] is generalized to L-stage reducible theories. The dependence of the generating functional of Green's functions on the choice of gauge in the massive case is dicussed and Ward identities related to osp(1,2) symmetry are given. Massive first stage theories with closed gauge algebra are studied in detail. The generalization of the Chapline-Manton model and topological Yang-Mills theory to the case of massive fields is consedered as examples.
description: 24 pages, AMSTEX, some minor improvements, 2 additional references
Effect of Coulomb Interactions on the Electronic and Magnetic Properties of Two-Dimensional CrSiTe$_3$ and CrGeTe$_3$ Materials
Creators: name: Kang, Sungmo
name: Kang, Seungjin
name: Yu, Jaejun
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate the electronic and magnetic structures of two-dimensional transition metal tri-chalcogenide CrSiTe$_{3}$ and CrGeTe$_{3}$ materials by carrying out first-principles calculations. The single-layer CrSiTe$_3$ and CrGeTe$_3$ are found to be a ferromagnetic insulator, where the presence of the strong $dpσ$-hybridization of Cr $e_{\mathrm{g}}$-Te $p$ plays a crucial role for the ferromagnetic coupling between Cr ions. We observe that the bandgaps and the interlayer magnetic order vary notably depending on the magnitude of on-site Coulomb interaction $U$ for Cr $d$ electrons. The bandgaps are formed between the Cr $e_{\mathrm{g}}$ conduction bands and the Te $p$ valence bands for both CrSiTe$_3$ and CrGeTe$_3$ in the majority-spin channel. The dominant Te $p$ antibonding character in the valence bands just below the Fermi level is related to the decrease of the bandgap for the increase of $U$. We elucidate the energy band diagram, which may serve to understand the electronic and magnetic properties of the $ABX_3$-type transition metal tri-chalcogenides in general.
description: 4 pages, 3 figures
The Hot Big Bang and Beyond
Creators: name: Turner, Michael S.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The hot big-bang cosmology provides a reliable accounting of the Universe from about $10^{-2}\sec$ after the bang until the present, as well as a robust framework for speculating back to times as early as $10^{-43}\sec$. Cosmology faces a number of important challenges; foremost among them are determining the quantity and composition of matter in the Universe and developing a detailed and coherent picture of how structure (galaxies, clusters of galaxies, superclusters, voids, great walls, and so on) developed. At present there is a working hypothesis---cold dark matter---which is based upon inflation and which, if correct, would extend the big bang model back to $10^{-32}\sec$ and cast important light on the unification of the forces. Many experiments and observations, from CBR anisotropy experiments to Hubble Space Telescope observations to experiments at Fermilab and CERN, are now putting the cold dark matter theory to the test. At present it appears that the theory is viable only if the Hubble constant is smaller than current measurements indicate (around $30\kms\Mpc^{-1}$), or if the theory is modified slightly, e.g., by the addition of a cosmological constant, a small admixture of hot dark matter ($5\eV$ ``worth of neutrinos''), more relativistic particles, or a tilted spectrum of density perturbations.
description: Summary of a talk given at IAU 168 and CAM-94; revised version contains part of abstract that was missing in original
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0451
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/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0451, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0451, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Introduction to AI-READI, Studying Salutogenesis in T2DM (dkNET Presentation)
Creators: name: Lee, Cecilia
name: Patel, Bhavesh
name: Baxter, Sally
Publisher: name: Zenodo
Year: 2024
Subjects: subject: Salutogenesis
subject: Type 2 Diabetes
subject: Diabetes
subject: AI-ready
subject: FAIR Data

description: The Abstract of the talk is provided below. More information is available at https://dknet.org/about/webinar.

Abstract

The AI-READI (Artificial Intelligence Ready and Equitable Atlas for Diabetes Insights, https://aireadi.org) project, funded by the NIH Common Fund’s Bridge2AI Program, aims to develop a multimodal dataset specifically designed to be AI-ready for the study of salutogenesis in Type 2 Diabetes Mellitus (T2DM). Despite advancements in diabetes care, limited knowledge exists on how individuals with T2DM may revert to health. AI-READI team is building this dataset from a diverse cohort of 4,000 participants, ensuring it is structured for immediate use in machine learning algorithm training and analysis. The project emphasizes ethical and equitable data collection, adherence to FAIR (Findable, Accessible, Interoperable, Reusable) data principles, and establishing best practices for data sharing and management. By focusing on AI-readiness, the dataset will enable rapid application of machine learning to uncover novel insights into effective treatment strategies.

This presentation will introduce the AI-READI project, present the dataset, demonstrate how to request the datasets and explore potential research questions that can be addressed using machine learning, such as identifying predictors of health improvement in T2DM, understanding disease progression, and investigating the impact of various risk factors.

The top 3 key questions that Bridge2AI AI-READI datasets can answer:

How can we better understand Type 2 Diabetes (T2DM) heterogeneity?

What are the connections between multi-organ function in T2DM, and how are the kidney, heart, eye, brain interlinked?

How do interactions between environmental factors (e.g. air pollution) drive outcomes in T2DM?
Cataulacus pygmaeus André, 1890, nov. sp.
Creators: name: André, E.
Publisher: name: Zenodo
Year: 1890
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Cataulacus
Cataulacus pygmaeus

description: Cataulacus pygmaeus nov. sp.
Ouvriere: Tete a peu pres aussi longue que large, retrecie en avant, avec le bord posterieur presque recliligne et denticule pres de ses angles ainsi que la moitie posterieure des bords lateraux. Epistome sans limites distinctes, tres faiblement echancre au milieu de son bord anterieur, muni d'une petite dent relevee a chacun de ses angles anterieurs qui prolongent les aretes frontales; ces dernieres portent elles-memes un petit denticule en avant des yeux. Yeux grands, situes derriere le milieu de la tete. Scape des antennes arque, tres dilate sur sa seconde moitie; funicule avec une massue. epaisse de trois articles. Thorax plus long que large, sans sutures entre ses divers segments, irregulierement trapezoidal et plus large en avant qu'en arriere; son profil dorsal est legerement convexe et non sensiblement sinue entre le mesonotum et le metanotum; ses bords lateraux sont denticules et il est muni en arriere de deux appendices spiniformes, divergents, tronques a l'extremite et un peu moins longs que la largeur du metanotum. Les deux articles du petiole trapeciformes, plus larges en avant qu'en arriere; le premier a peu pres aussi long que large, le second un peu plus large que long et muni en dessous d'une epine mousse. Abdomen ovale, avec le bord anterieur fortement echancre en arc.
Entierement noire, avec l'extremite des mandibules, le funicule iles antennes et les articulations des pattes d'un rouge plus ou moins brun; scapes, tibias et tarses d'un jaune rougeatre.
Tete avec des rides longitudinales qui se reunissent, surtout en arriere, a de petites rides transversales pour former un reseau de moilles irregulieres dont le fond est lui-meme plus finement reti- cule. Thorax avec des rides longitudinales plus fortes, reticule, dans les intervalles et parseme d'elevations granuleuses. Petiole tres fortement et longitudinalement ride-sillonne, le second article parseme d'elevations en forme de denticules. Abdomen densement et finement reticule-ponctue, avec de petites elevations granuleuses tres eparses. Tout le corps, y compris les antennes et les pattes, parseme de soies jaunatres, courtes, obtuses a l'extremite et peu abondantes.
Long., un peu plus de 2 mill.
Un seul-individu.
Cette espece se rapproche, pour l'aspect general, du C. guineensis Sm., mais elle en est bien distincte par son thorax depourvu d'epines laterales, par les epines de son metanotum moins longues et plus obtuses, par son abdomen non ride longitudinalement et par sa taille extremement petite.
description: Published as part of André, E., 1890, Matériaux pour servir a la faune myrmécologique de Sierra-Leone (Afrique occidentale)., pp. 311-327 in Revista de Entomologia 9 on pages 325-326
Spin liquid fingerprints in the thermal transport of a Kitaev-Heisenberg ladder
Creators: name: Metavitsiadis, Alexandros
name: Psaroudaki, Christina
name: Brenig, Wolfram
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We identify fingerprints of a proximate quantum spin-liquid (QSL), observable by finite-temperature dynamical thermal transport within a minimal version of the idealized Kitaev model on a two-leg ladder, if subjected to inevitably present Heisenberg couplings. Using exact diagonalization and quantum typicality, we uncover (i) an insulator-conductor crossover induced by fracton recombination at infinitesimal Heisenberg coupling, (ii) low- and high-energy signatures of fractons, which survive far off the pure QSL point, and (iii) a non-monotonous current life-time versus Heisenberg couplings. Guided by perturbation theory, we find (iv) a Kitaev-exchange induced `one-magnon' contribution to the dynamical heat transport in the strong Heisenberg rung limit.
description: 6 pages, 4 figures. See also ancillary files
Gauge dependence and matching procedure of a nonrelativistic QED/QCD boundstate formalism
Creators: name: Hasebe, K.
name: Sumino, Y.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A nonrelativistic boundstate formalism used in contemporary calculations is investigated. It is known that the effective Hamiltonian of the boundstate system depends on the choice of gauge. We obtain the transformation charge Q of the Hamiltonian for an arbitrary infinitesimal change of gauge, by which gauge independence of the mass spectrum and gauge dependences of the boundstate wave functions are dictated. We give formal arguments based on the BRST symmetry supplemented by power countings of Coulomb singularities of diagrams. For illustration: (1)we calculate Q up to O(1/c), (2)we examine gauge dependences of diagrams for a decay of a qqbar boundstate up to O(1/c) and show that cumbersome gauge cancellations can be circumvented by directly calculating Q. As an application we point out that the present calculations of top quark momentum distribution in the ttbar threshold region are gauge dependent. We also show possibilities for incorrect calculations of physical quantities of boundstates when the on-shell matching procedure is employed. We give a proof of a justification for the use of the equation of motion to simplify the form of a local NRQCD Lagrangian. The formalism developed in this work will provide useful cross checks in computations involving NRQED/NRQCD boundstates.
description: 30 pages, 15 figures (ver1); Presentations of Introduction and Conclusion were modified substantially, although none of our findings have been changed; Side remarks have been added in various parts of the paper. (ver2); Supplementary remarks and minor corrections (ver3)
Braneworld in $f(T)$ Gravity Theory with Noncanonical Scalar Matter Field
Creators: name: Wang, Jian
name: Guo, Wen-Di
name: Lin, Zi-Chao
name: Liu, Yu-Xiao
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this paper, we investigate the braneworld scenario in $f(T)$ gravity with a $K$-field as the background field. We consider various different specific forms of $f(T)$ gravity and $K$-field, and find a general way to construct the braneworld model. Based on our solutions, the split of branes is investigated. Besides, the stability of the braneworld is studied by investigating the tensor perturbation of the vielbein.
description: v3: 11 pages, 6 figures, updated version, accepted by PRD
Additional file 1: of Heterogeneous burden of lung disease in smokers with borderline airflow obstruction
Creators: name: Pirozzi, Cheryl
name: Gu, Tian
name: Quibrera, Pedro
name: Carretta, Elizabeth
name: Han, MeiLan
name: Murray, Susan
name: Cooper, Christopher
name: Tashkin, Donald
name: Kleerup, Eric
name: Barjaktarevic, Igor
name: Hoffman, Eric
name: Martinez, Carlos
name: Christenson, Stephanie
name: Hansel, Nadia
name: R. Graham Barr
name: Bleecker, Eugene
name: Ortega, Victor
name: Martinez, Fernando
name: Kanner, Richard
name: Paine, Robert
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: Science Policy

description: Table S1. Baseline characteristics for the four groups. Table S2. Comparison of physiologic and clinical variables between ever-smokers with normal FEV1 and FEV1/FVC > LLN but 0.70 (Group 2), never-smokers with normal FEV1 and FEV1/FVC > 0.70 (Group 3) and ever-smokers with FEV1/FVC ≤ LLN and > 75th quartile (Group 4). Table S3. Comparison of CT variables between ever-smokers with normal FEV1 and FEV1/FVC > LLN but 0.70 (Group 2), never-smokers with normal FEV1 and FEV1/FVC > 0.70 (Group 3) and ever-smokers with FEV1/FVC ≤ LLN and > 75th quartile (Group 4). (DOCX 100 kb)
The Importance of Realistic Starting Models for Hydrodynamic Simulations of Stellar Collisions
Creators: name: Sills, Alison
name: Lombardi, James C.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We demonstrate the necessity of using realistic stellar models taken from stellar evolution codes, as opposed to polytropes, for starting models in smoothed particle hydrodynamics calculations of collisions between main sequence stars. Evolved stars have mean molecular weight gradients, which affect their entropy profiles and therefore affect how they react during a collision. The structure of stellar collision products of polytrope parent stars is significantly different from that of collision products of realistic parent models. These differences strongly affect the future evolution of the collision products, particularly products of collisions between unequal mass stars which have undergone significant chemical evolution. The use of polytropes as parent star models is likely to result in qualitatively mistaken results for the structure of the collision product.
description: 13 pages, 4 encapsulated postscript figures, accepted by Astrophysical Journal (Letters)
Relaminarising pipe flow by wall movement
Creators: name: Scarselli, Davide
name: Kühnen, Jakob
name: Hof, Björn
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Following the recent observation that turbulent pipe flow can be relaminarised by a relatively simple modification of the mean velocity profile, we here carry out a quantitative experimental investigation of this phenomenon. Our study confirms that a flat velocity profile leads to a collapse of turbulence and in order to achieve the blunted profile shape, we employ a moving pipe segment that is briefly and rapidly shifted in the streamwise direction. The relaminarisation threshold and the minimum shift length and speeds are determined as a function of Reynolds number. Although turbulence is still active after the acceleration phase, the modulated profile possesses a severely decreased lift-up potential as measured by transient growth. As shown, this results in an exponential decay of fluctuations and the flow relaminarises. While this method can be easily applied at low to moderate flow speeds, the minimum streamwise length over which the acceleration needs to act increases linearly with the Reynolds number.
description: 13 pages, 9 figures
Constraints on a Parity-even/Time-Reversal-odd Interaction
Creators: name: van Oers, Willem T. H.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Time-Reversal-Invariance non-conservation has for the first time been unequivocally demonstrated in a direct measurement, one of the results of the CPLEAR experiment. What is the situation then with regard to time-reversal-invariance non-conservation in systems other than the neutral kaon system? Two classes of tests of time-reversal-invariance need to be distinguished: the first one deals with parity violating (P-odd)/time-reversal-invariance non-conserving (T-odd) interactions, while the second one deals with P-even/T-odd interactions (assuming CPT conservation this implies C-conjugation non-conservation). Limits on a P-odd/T-odd interaction follow from measurements of the electric dipole moment of the neutron. This in turn provides a limit on a P-odd/T-odd pion-nucleon coupling constant which is 10^-4 times the weak interaction strength. Limits on a P-even/T-odd interaction are much less stringent. The better constraint stems also from the measurement of the electric dipole moment of the neutron. Of all the other tests, measurements of charge-symmetry breaking in neutron-proton elastic scattering provide the next better constraint. The latter experiments were performed at TRIUMF (at 477 and 347 MeV) and at IUCF (at 183 MeV). Weak decay experiments (the transverse polarization of the muon in K+ -> pi0 mu+ nu and the transverse polarization of the positrons in polarized muon decay) have the potential to provide comparable or possibly better constraints.
description: 7 Pages LaTeX, 2 PostScript figures, uses aipproc.sty. Written version of Invited Paper presented at the 3rd International Symposium on Symmetries in Subatomic Physics, Adelaide, SA, Australia, March 13-17, 2000
ChEMBL dense datasets for DL/ML binding affinity prediction
Creators: name: Gómez-Tamayo, Jose Carlos
Publisher: name: Zenodo
Year: 2024

description: High-quality dense protein-ligand complexes for 6 protein targets (ABL, BACE1, MAPK, VEGF, EGFR, PLK1) extracted from chEMBL. These datasets aim to improve 3D DL/ML binding affinity precition models by adding dense information capturing SAR from hundreds/thousands of molecules binding to the same pocket.
Myrmecia picta Sm.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1900
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Myrmecia
Myrmecia picta

description: Myrmecia picta Sm.
[[worker]]. - Perth, Australie occid. (Chase). - L'exemplaire [[worker]] n'a que 5,8 mill. Tandis que le metanotum est rouge, comme chez certains exemplaires du Queensland, dont parle Mayr, les pattes, les antennes et la plus grande partie des mandibules sont entierement d'un bran sale. Je crois que cette variete merite d'etre fixee (var. infima n. var.).
description: Published as part of Forel, A., 1900, Ponerinae et Dorylinae d'Australie. Récoltés par MM. Turner, Froggatt, Nugent, Chase, Rothney, J. - J. Walker, etc., pp. 54-77 in Annales de la Societe Entomologique de Belgique 44 on page 54
Wigner functions in covariant and single-time formulations
Creators: name: Ochs, Stefan
name: Heinz, Ulrich
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We will establish the connection between the Lorentz covariant and so-called single-time formulation for the quark Wigner operator. To this end we will discuss the initial value problem for the Wigner operator of a field theory and give a discussion of the gauge-covariant formulation for the Wigner operator including some new results concerning the chiral limit. We discuss the gradient or semi-classical expansion and the color and spinor decomposition of the equations of motion for the Wigner operator. The single-time formulation will be derived from the covariant formulation by taking energy moments of the equations for the Wigner operator. For external fields we prove that only the lowest energy moments of the quark Wigner operator contain dynamical information.
description: 92 pages, to appear in Annals of Physics (N.Y.)
Additional file 1: of Mothersâ and fatherâ s perceptions of the risks and benefits of screen time and physical activity during early childhood: a qualitative study
Creators: name: Hinkley, Trina
name: McCann, Jennifer
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Interview schedule. (DOCX 14 kb)
Pulse Morphology of the Galactic Center Magnetar PSR J1745-2900
Creators: name: Pearlman, Aaron B.
name: Majid, Walid A.
name: Prince, Thomas A.
name: Kocz, Jonathon
name: Horiuchi, Shinji
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present results from observations of the Galactic Center magnetar, PSR J1745-2900, at 2.3 and 8.4 GHz with the NASA Deep Space Network 70 m antenna, DSS-43. We study the magnetar's radio profile shape, flux density, radio spectrum, and single pulse behavior over a ~1 year period between MJDs 57233 and 57621. In particular, the magnetar exhibits a significantly negative average spectral index of $\langleα\rangle$ = -1.86 $\pm$ 0.02 when the 8.4 GHz profile is single-peaked, which flattens considerably when the profile is double-peaked. We have carried out an analysis of single pulses at 8.4 GHz on MJD 57479 and find that giant pulses and pulses with multiple emission components are emitted during a significant number of rotations. The resulting single pulse flux density distribution is incompatible with a log-normal distribution. The typical pulse width of the components is ~1.8 ms, and the prevailing delay time between successive components is ~7.7 ms. Many of the single pulse emission components show significant frequency structure over bandwidths of ~100 MHz, which we believe is the first observation of such behavior from a radio magnetar. We report a characteristic single pulse broadening timescale of $\langleτ_{d}\rangle$ = 6.9 $\pm$ 0.2 ms at 8.4 GHz. We find that the pulse broadening is highly variable between emission components and cannot be explained by a thin scattering screen at distances $\gtrsim$ 1 kpc. We discuss possible intrinsic and extrinsic mechanisms for the magnetar's emission and compare our results to other magnetars, high magnetic field pulsars, and fast radio bursts.
description: 18 pages, 12 figures, Accepted for publication in ApJ on 2018 August 30. v2: Updated to match published version
Design optimization of a lightweight secondary mirror assembly for a 1-m class ground telescope for satellite laser ranging
Creators: name: Lee, Jaehyun
name: Park, Kisoo
name: Son, Eui Seung
name: Jeong, Suseong
name: Kim, Do-Won
name: Oh, Han-Gyol
name: Kang, Pilseong
name: Rhee, Hyug-Gyo
Publisher: name: Taylor & Francis
Year: 2025
Subjects: Biophysics
Space Science
Physical Sciences not elsewhere classified
Medicine
Biotechnology
Environmental Sciences not elsewhere classified
Chemical Sciences not elsewhere classified

description: Large-sized ground telescopes have been developed to meet the high demands for opto-mechanical imaging systems in space and military applications. In line with these advancements, we developed a 1-m class ground telescope for astronomical imaging and satellite laser ranging (SLR). In a ground telescope, mirror deflection is mainly induced by gravity and temperature change. In particular, the gravity vector varies depending on the pointing direction of a telescope, so the surface deformations of the mirrors due to self-gravity need to be managed in different observation directions. This study introduces a mechanical design for an optical tube assembly (OTA) and suggests an optimized design for the secondary mirror (M2) assembly. For a kinematic positioning of the M2, its lightweight was achieved based on the partially open-back structure with hexagonal pocket cells. Then, we optimized the flexure mount design with a bipod structure to minimize the surface errors (SFEs) of the M2 in both the horizontal and vertical pointing directions. Additionally, we simulated the deflections of the primary mirror (M1) and M2 assemblies when installed on the telescope. Based on our design, the M2 was fabricated and processed, and we demonstrated its assembly process and surface quality test.
Evaluating radiation transport errors in merger simulations using a Monte-Carlo algorithm
Creators: name: Foucart, Francois
name: Duez, Matthew D.
name: Kidder, Lawerence E.
name: Nguyen, Ronny
name: Pfeiffer, Harald P.
name: Scheel, Mark A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Neutrino-matter interactions play an important role in the post-merger evolution of neutron star-neutron star and black hole-neutron star mergers. Most notably, they determine the properties of the bright optical/infrared transients observable after a merger. Unfortunately, Boltzmann's equations of radiation transport remain too costly to be evolved directly in merger simulations. Simulations rely instead on approximate transport algorithms with unquantified modeling errors. In this paper, we use for the first time a time-dependent general relativistic Monte-Carlo (MC) algorithm to solve Boltzmann's equations and estimate important properties of the neutrino distribution function ~10ms after a neutron star merger. We do not fully couple the MC algorithm to the fluid evolution, but use a short evolution of the merger remnant to critically assess errors in our approximate gray two-moment transport scheme. We demonstrate that the analytical closure used by the moment scheme is highly inaccurate in the polar regions, but performs well elsewhere. While the average energy of polar neutrinos is reasonably well captured by the two-moment scheme, estimates for the neutrino energy become less accurate at lower latitudes. The two-moment formalism also overestimates the density of neutrinos in the polar regions by ~50%, and underestimates the neutrino pair-annihilation rate at the poles by factors of 2-3. Although the latter is significantly more accurate than one might have expected before this study, our results indicate that predictions for the properties of polar outflows and for the creation of a baryon-free region at the poles are likely to be affected by errors in the two-moment scheme, thus limiting our ability to reliably model kilonovae and gamma-ray bursts.
description: 15 pages, 10 figures