cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MOESM2 of Pelagibaca bermudensis promotes biofuel competence of Tetraselmis striata in a broad range of abiotic stressors: dynamics of quorum-sensing precursors and strategic improvement in lipid productivity
Creators: name: Shailesh Patidar
name: Sae-Hee Kim
name: Kim, Jin
name: Jungsoo Park
name: Park, Bum
name: Han, Myung-Soo
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Molecular Biology
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: Inorganic Chemistry

description: Additional file 2: Table S1. Post hoc t analysis for comparison of means (LSD) based on one-way ANOVA results of the data shown in Figs.Â 1 and 5 (Biomass productivity and total lipid content under different environmental variables and two-stage cultivation); (Table Aâ H).
Towards Long-endurance Flight: Design and Implementation of a Variable-pitch Gasoline-engine Quadrotor
Creators: name: Pang, T.
name: Peng, K.
name: Lin, F.
name: Chen, B. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: Majority of today's fixed-pitch, electric-power quadrotors have short flight endurance ($
description: 6 pages
Couplings varying on cosmological scales and Lorentz breaking
Creators: name: Lehnert, Ralf
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the context of N=4 supergravity in four dimensions, we present an exact classical solution that leads to spacetime-dependent electromagnetic couplings and discuss the ensuing Lorentz-violating effects. We comment briefly on experimental bounds.
description: 10 pages, 1 figure, invited talk presented at the Coral Gables Meeting, December 2002
Clematis cirrhosa Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Clematis
Clematis cirrhosa

description: Clematis cirrhosa, spec. nov.
 6. Clematis cirrhis scandens. Hort. cliff. 226. Roy. lugdb. 487.
 Clematitis peregrina, foliis pyri incisis. Bauh. pin. 300.
 Clematis altera baetica. Clus. hist. 1. p. 123.
 Clematis peregrina, foliis pyri incisis: nunc singularibus, nunc ternis. Tournef. cor.20.
 Habitat in Baetica , arbores operiens & deprimens.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 544, DOI: 10.5281/zenodo.3931989
Mid- and high-J CO observations towards UCHIIs
Creators: name: Wyrowski, F.
name: Heyminck, S.
name: Guesten, R.
name: Menten, K. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A study of 12 ultracompact HII regions was conducted to probe the physical conditions and kinematics in the inner envelopes of the molecular clumps harboring them. The APEX telescope was used to observe the sources in the CO (4-3) and 13CO (8-7) lines. Line intensities were modeled with the RATRAN radiative transfer code using power laws for the density and temperature to describe the physical structure of the clumps. All sources were detected in both lines. The optically thick CO (4-3) line shows predominantly blue skewed profiles reminiscent of infall. Line intensities can be reproduced well using the physical structure of the clumps taken from the literature. The optically thick line profiles show that CO is a sensitive tracer of ongoing infall in the outer envelopes of clumps harboring ultracompact HII regions and hot molecular cores.
description: APEX A&A special issue, accepted
Supplementary Material 6: from Mechanistic models for West Nile virus transmission: a systematic review of features, aims and parametrization
Creators: name: de Wit, Mariken
name: Martins, Afonso Dimas
name: Delecroix, Clara
name: Heesterbeek, Hans
name: ten Bosch, Quirine
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310299
subject: Bioinformatics and computational biology not elsewhere classified
classificationCode: 310399
subject: Ecology not elsewhere classified
classificationCode: 420299
subject: Epidemiology not elsewhere classified

description: Variation in parameters estimates based on the most cited empirical study
Additional file 2: of Examining the challenges posed to parents by the contemporary screen environments of children: a qualitative investigation
Creators: name: Solomon-Moore, Emma
name: Matthews, Joe
name: Reid, Thomas
name: Toumpakari, Zoi
name: Sebire, Simon
name: Thompson, Janice
name: Lawlor, Deborah
name: Jago, Russell
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Table S1. Parents’ descriptions of their child’s weekend SV time compared to numerate levels reported in questionnaire. A table displaying parents’ descriptions of their child’s weekend screen viewing time compared to numerate levels reported in the questionnaire. (DOCX 13 kb)
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00181
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00181, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Towards understanding $b\bar{b}$ production in $γγ$ collisions
Creators: name: Chyla, Jiri.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Understanding the data on the total cross section $σ_{tot}($e$^+$e$^-\to$e$^+$e$^-b\bar{b})$ measured at LEP2 represents a serious challenge for perturbative QCD. In order to unravel the origins of the discrepancy between data and theory, we investigate the dependence of four contributions to this cross section on $γγ$ collision energy. As the reliability of the existing calculations of $σ_{tot}($e$^+$e$^-\to$e$^+$e$^-b\bar{b})$ depends, among other things, on the stability of calculations of the cross section $σ_{tot}(γγ\to b\bar{b})$ with respect to variations of the renormalization and factorization scales, we investigate this aspect in detail. We show that in most of the region relevant for the LEP2 data the existing QCD calculations of $σ_{tot}(γγ\to b\bar{b})$ do not exhibit a region of local stability and should thus be taken with caution. The source of this instability is suggested and its phenomenological implications for LEP2 data are discussed.
description: 16 pages, latex with 10 eps-figures, misprints corrected, some formulations amended
Disproval of the validated planets K2-78b, K2-82b, and K2-92b
Creators: name: Cabrera, J.
name: Barros, S. C. C.
name: Armstrong, D.
name: Hidalgo, D.
name: Santos, N. C.
name: Almenara, J. M.
name: Alonso, R.
name: Deleuil, M.
name: Demangeon, O.
name: Diaz, R. F.
name: Lendl, M.
name: Pfaff, J.
name: Rauer, H.
name: Santerne, A.
name: Serrano, L. M.
name: Zucker, S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Transiting super-Earths orbiting bright stars in short orbital periods are interesting targets for the study of planetary atmospheres. While selecting super-Earths suitable for further characterization from the ground among a list of confirmed and validated exoplanets detected by K2, we found some suspicious cases that led to us re-assessing the nature of the detected transiting signal. We did a photometric analysis of the K2 light curves and centroid motions of the photometric barycenters. Our study shows that the validated planets K2-78b, K2-82b, and K2-92b are actually not planets but background eclipsing binaries. The eclipsing binaries are inside the Kepler photometric aperture, but outside the ground-based high resolution images used for validation. We advise extreme care on the validation of candidate planets discovered by space missions. It is important that all the assumptions in the validation process are carefully checked. An independent confirmation is mandatory in order to avoid wasting valuable resources on further characterization of non-existent targets.
description: accepted for publication in A&A
Supplementary Material 1: from Mechanistic models for West Nile virus transmission: a systematic review of features, aims and parametrization
Creators: name: de Wit, Mariken
name: Martins, Afonso Dimas
name: Delecroix, Clara
name: Heesterbeek, Hans
name: ten Bosch, Quirine
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310299
subject: Bioinformatics and computational biology not elsewhere classified
classificationCode: 310399
subject: Ecology not elsewhere classified
classificationCode: 420299
subject: Epidemiology not elsewhere classified

description: Systematic database search routine
Clematis integrifolia Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Clematis
Clematis integrifolia

description: Clematis integrifolia, spec. nov.
 9. Clematis foliis simplicibus ovato-lanceolatis. Hort. cliff. 225. Hort. ups. 156. Roy. lugdb. 486.
 Clematitis caerulea erecta. Bauh. pin. 300.
 Clematis caerulea pannonica. Clus. hist. 1. p. 123.
 Habitat in Hungaria , Tataria . ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on pages 544-545, DOI: 10.5281/zenodo.3931989
MOESM1 of The effect of change in fasting glucose on the risk of myocardial infarction, stroke, and all-cause mortality: a nationwide cohort study
Creators: name: Gyeongsil Lee
name: Kim, Sung
name: Seulggie Choi
name: Kyuwoong Kim
name: Jeong, Su-Min
name: Son, Joung
name: Jae-Moon Yun
name: Park, Sang
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 1: Table S1. Associations between change in fasting glucose from the first health examination and the risk of myocardial infarction, stroke, and all-cause mortality excluding participants whose myocardial infarction, stroke, or death occurred in from January 1, 2006 to December 31, 2006. Table S2. Associations between change in fasting glucose at the first health examination and the risk of myocardial infarction, stroke, and all-cause mortality excluding participants whose myocardial infarction, stroke, or death occurred in from January 1, 2006 to December 31, 2007.
Thalictrum alpinum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Thalictrum
Thalictrum alpinum

description: Thalictrum alpinum, spec. nov.
 1. Thalictrum caule simplicissimo subnudo, racemo simplici terminali. Hort. cliff. 227. Fl. suec. 455. Roy. lugdb. 485.
 Thalictrum caule subnudo simplici, foliolis obtusis. Fl. lapp. 225. *
 Thalictrum montanum minimum praecox, foliis splendentibus. Moris. hist. 3. p.325. s.9. t.20. f.14.
 Habitat in Alpibus Lapponiae , Arvoniae . ♃
 Petala 4, Stamina 12, Pistilla 8, Racemus simplex floribus cernuis.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 545, DOI: 10.5281/zenodo.3931989
title: ADCO, Second cartulaire de Saint-Étienne de Dijon (XVe siècle), Cart. 22 (G 126), 110 folios, f. 0017
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Second cartulaire de Saint-Étienne de Dijon (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 22 (G 126), 110 folios, f. 0017, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Second cartulaire de Saint-Étienne de Dijon (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 22 (G 126), 110 folios, f. 0017, 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
The algebra of knotted trivalent graphs and Turaev's shadow world
Creators: name: Thurston, Dylan P.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Geometric Topology (math.GT)
subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics
subject: 57M25, 57M20, 57Q40

description: Knotted trivalent graphs (KTGs) form a rich algebra with a few simple operations: connected sum, unzip, and bubbling. With these operations, KTGs are generated by the unknotted tetrahedron and Moebius strips. Many previously known representations of knots, including knot diagrams and non-associative tangles, can be turned into KTG presentations in a natural way. Often two sequences of KTG operations produce the same output on all inputs. These `elementary' relations can be subtle: for instance, there is a planar algebra of KTGs with a distinguished cycle. Studying these relations naturally leads us to Turaev's shadow surfaces, a combinatorial representation of 3-manifolds based on simple 2-spines of 4-manifolds. We consider the knotted trivalent graphs as the boundary of a such a simple spine of the 4-ball, and to consider a Morse-theoretic sweepout of the spine as a `movie' of the knotted graph as it evolves according to the KTG operations. For every KTG presentation of a knot we can construct such a movie. Two sequences of KTG operations that yield the same surface are topologically equivalent, although the converse is not quite true.
description: Published by Geometry and Topology Monographs at http://www.maths.warwick.ac.uk/gt/GTMon4/paper22.abs.html
Angular Momentum Transport in Thin Magnetically Arrested Disks
Creators: name: Marshall, Megan D.
name: Avara, Mark J.
name: McKinney, Jonathan C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In accretion disks with large-scale ordered magnetic fields, the magnetorotational instability (MRI) is marginally suppressed, so other processes may drive angular momentum transport leading to accretion. Accretion could then be driven by large-scale magnetic fields via magnetic braking, but large-scale magnetic flux can build-up onto the black hole and within the disk leading to a magnetically-arrested disk (MAD). Such a MAD state is unstable to the magnetic Rayleigh-Taylor (RT) instability, which itself leads to vigorous turbulence and the emergence of low-density highly-magnetized bubbles. This instability was studied in a thin (ratio of half-height H to radius R, $H/R \approx 0.1$) MAD simulation, where it has a more dramatic effect on the dynamics of the disk than for thicker disks. We find that the low-density bubbles created by the magnetic RT instability decrease the stress (leading to angular momentum transport) in the disk rather than increasing magnetic torques. Indeed, we find that the dominant component of the stress is due to turbulent magnetic fields, despite the suppression of the axisymmetric MRI and the dominant presence of large-scale magnetic fields. This suggests that the magnetic RT instability plays a significant role in driving angular momentum transport in MADs.
description: 7 pages, 6 figures. Movies: https://youtu.be/Sfh9O6Nm5Cc https://youtu.be/74CuoWN2HjI
Thalictrum foetidum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Thalictrum
Thalictrum foetidum

description: Thalictrum foetidum, spec. nov.
2. Thalictrum caule paniculato ramosissimo folioso.
 Thalictrum caule filiformi ramosissimo in paniculam disperso subjectis foliolis. Hort. cliff. 227. * Roy. lugdb. 485. Sauv. monsp. 251.
 Thalictrum minimum foetidissimum. Bauh. pin. 337. prodr. 147. Bauh. hist. 3. p.488. Moris. hist. 3. p.325. s.9. t.20. f.13. Pluk. alm. 367. t.65. f.4.
 Habitat Monspelii , inque Vallesia , Helvetia . ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 545, DOI: 10.5281/zenodo.3931989
MOESM1 of One-step ahead forecasting of geophysical processes within a purely statistical framework
Creators: name: Papacharalampous, Georgia
name: Tyralis, Hristos
name: Demetris Koutsoyiannis
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Additional file 1. Exploration of the datasets.
The Star Formation History of the Disk of the Starburst galaxy M82
Creators: name: Mayya, Y. D.
name: Bressan, A.
name: Carrasco, L.
name: Hernandez, L.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Spectroscopic, photometric and dynamical data of the inner 3 kpc part of the starburst galaxy M82 are analyzed in order to investigate the star formation history of the stellar disk. The long-slit spectra along the major axis are dominated by Balmer absorption lines in the region outside the nuclear starburst all the way up to ~3.5 scalelengths (mu_B=22 mag/arcsec**2). Single Stellar Population (SSP) spectra of age 0.4-1.0 Gyr match well the observed spectra in the 1-3 kpc zone, with a mean age of the stellar population marginally higher in the outer parts. The mass in these populations, along with that in the gas component, make up for the inferred dynamical mass in the same annular zone for a Kroupa initial mass function, with a low mass cut-off m_l=0.4 Msun. The observed ratio of the abundances of alpha elements with respect to Fe, is also consistent with the idea that almost all the stars in M82 disk formed in a burst of short duration (0.3 Gyr) around 0.8 Gyr ago. We find that the optical/near infrared colors and their gradients in the disk are determined by the reddening with visual extinction exceeding 1 mag even in the outer parts of the disk, where there is apparently no current star formation. The disk-wide starburst activity was most likely triggered by the interaction of M82 with its massive neighbor M81 around 1~Gyr ago. The properties of the disk of M82 very much resemble the properties of the disks of luminous compact blue galaxies seen at 0.2-1.0 redshift.
description: 7 pages, Accepted for publication in ApJ
Thalictrum tuberosum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Thalictrum
Thalictrum tuberosum

description: Thalictrum tuberosum, spec. nov.
 3. Thalictrum floribus pentapetalis, radice tuberosa. Hort. cliff. 227. Roy. lugdb. 486.
 Thalictrum minus, asphodeli radice, magno flore. Tournef. inst. 271.
 Ranunculus thalictri folio, asphodeli radice. Moris. hist. 2. p.438. s.4. t.28. f.13.
 Oenanthe folio hederae. Bauh. pin. 163.
 Habitat in Hispania . ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 545, DOI: 10.5281/zenodo.3931989
A few remarks about symplectic filling
Creators: name: Eliashberg, Yakov
Publisher: name: arXiv
Year: 2003
Subjects: subject: Symplectic Geometry (math.SG)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 53C15, 57M50

description: We show that any compact symplectic manifold (W,ω) with boundary embeds as a domain into a closed symplectic manifold, provided that there exists a contact plane ξon dW which is weakly compatible with omega, i.e. the restriction ω|ξdoes not vanish and the contact orientation of dW and its orientation as the boundary of the symplectic manifold W coincide. This result provides a useful tool for new applications by Ozsvath-Szabo of Seiberg-Witten Floer homology theories in three-dimensional topology and has helped complete the Kronheimer-Mrowka proof of Property P for knots.
description: Published by Geometry and Topology at http://www.maths.warwick.ac.uk/gt/GTVol8/paper6.abs.html
Improving time-delay cosmography with spatially resolved kinematics
Creators: name: Shajib, Anowar J.
name: Treu, Tommaso
name: Agnello, Adriano
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Strongly gravitational lensed quasars can be used to measure the so-called time-delay distance $D_{Δt}$, and thus the Hubble constant $H_0$ and other cosmological parameters. Stellar kinematics of the deflector galaxy play an essential role in this measurement by: (i) helping break the mass-sheet degeneracy; (ii) determining in principle the angular diameter distance $D_{\rm d}$ to the deflector and thus further improving the cosmological constraints. In this paper we simulate observations of lensed quasars with integral field spectrographs and show that spatially resolved kinematics of the deflector enable further progress by helping break the mass-anisotropy degeneracy. Furthermore, we use our simulations to obtain realistic error estimates with current/upcoming instruments like OSIRIS on Keck and NIRSPEC on the James Webb Space Telescope for both distances (typically $\sim6$ per cent on $D_{Δt}$ and $\sim10$ per cent on $D_{\rm d}$). We use the error estimates to compute cosmological forecasts for the sample of nine lenses that currently have well measured time delays and deep Hubble Space Telescope images and for a sample of 40 lenses that is projected to be available in a few years through follow-up of candidates found in ongoing wide field surveys. We find that $H_0$ can be measured with 2 per cent (1 per cent) precision from nine (40) lenses in a flat $Λ$cold dark matter cosmology. We study several other cosmological models beyond the flat $Λ$cold dark matter model and find that time-delay lenses with spatially resolved kinematics can greatly improve the precision of the cosmological parameters measured by cosmic microwave background data.
description: 18 pages, 11 figures, 7 tables, published in MNRAS (this version: added minor edits and some references as in the published version)
Frustration-induced internal stresses are responsible for quasilocalized modes in structural glasses
Creators: name: Lerner, Edan
name: Bouchbinder, Eran
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: It has been recently shown [E. Lerner, G. Düring, and E. Bouchbinder, Phys. Rev. Lett. 117, 035501 (2016)] that the non-phononic vibrational modes of structural glasses at low-frequencies $ω$ are quasi-localized and follow a universal density of states $D(ω)\!\sim\!ω^4$. Here we show that the gapless nature of the observed density of states depends on the existence of internal stresses which generically emerge in glasses due to frustration, thus elucidating a basic element underlying this universal behavior. Similarly to jammed particulate packings, low-frequency modes in structural glasses emerge from a balance between a local elasticity term and an internal stress term in the dynamical matrix, where the difference between them is orders of magnitude smaller than their typical magnitude. By artificially reducing the magnitude of internal stresses in a computer glass former in three dimensions, we show that a gap is formed in the density of states below which no vibrational modes exist, thus demonstrating the crucial importance of internal stresses. Finally, we show that while better annealing the glass upon cooling from the liquid state significantly reduces its internal stresses, the self-organizational processes during cooling render the gapless $D(ω)\!\sim\!ω^4$ density of state unaffected.
description: 4 pages, 3 figures. v2: New panel added to Fig.2 + additional references. v3: Fig.3 corrected + minor text additions
Following the Cosmic Evolution of Pristine Gas II: The search for Pop III-Bright Galaxies
Creators: name: Sarmento, Richard
name: Scannapieco, Evan
name: Cohen, Seth
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Direct observational searches for Population III (Pop III) stars at high redshift are faced with the question of how to select the most promising targets for spectroscopic follow-up. To help answer this, we use a large-scale cosmological simulation, augmented with a new subgrid model that tracks the fraction of pristine gas, to follow the evolution of high-redshift galaxies and the Pop III stars they contain. We generate rest-frame ultraviolet (UV) luminosity functions for our galaxies and find that they are consistent with current $z \ge 7 $ observations. Throughout the redshift range $7 \le z \le 15$ we identify "Pop III-bright" galaxies as those with at least 75% of their flux coming from Pop III stars. While less than 1% of galaxies brighter than $m_{\rm UV, AB} = 31.4$ mag are Pop III--bright in the range $7\leq z \leq8$, roughly 17% of such galaxies are Pop III--bright at $z=9$, immediately before reionization occurs in our simulation. Moving to $z=10$, $m_{\rm UV, AB} = 31.4$ mag corresponds to larger, more luminous galaxies and the Pop III-bright fraction falls off to 5%. Finally, at the highest redshifts, a large fraction (29% at $z=14$ and 41% at $z=15)$ of all galaxies are Pop III-bright regardless of magnitude. While $m_{\rm UV, AB} = 31.4$ mag galaxies are extremely rare during this epoch, we find that 13% of galaxies at $z = 14$ are Pop III-bright with $m_{\rm UV, AB} \le 33$ mag, an intrisic magnitude within reach of the James Webb Space Telescope using lensing. Thus, we predict that the best redshift to search for luminous Pop III--bright galaxies is just before reionization, while lensing surveys for fainter galaxies should push to the highest redshifts possible.
description: Accepted for publication by ApJ, Updated version with correct Figure 6
Additional file 1: of Examining the challenges posed to parents by the contemporary screen environments of children: a qualitative investigation
Creators: name: Solomon-Moore, Emma
name: Matthews, Joe
name: Reid, Thomas
name: Toumpakari, Zoi
name: Sebire, Simon
name: Thompson, Janice
name: Lawlor, Deborah
name: Jago, Russell
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: Computational Biology

description: Interview Guide. The interview guide used to conduct the qualitative interviews. (DOCX 29Â kb)
Thalictrum cornuti Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Thalictrum
Thalictrum cornuti

description: Thalictrum cornuti, spec. nov.
 4. Thalictrum floribus pentapetalis, radice fibrosa. Roy. lugdb. 486.
 Thalictrum canadense. Corn. canad. 186.
 Thalictrum americanum. Park. theatr. 265.
 Thalictrum majus, foliis aquilegiae, flore albo. Moris. hist. 3. p.325.
 Habitat in Canada . ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 545, DOI: 10.5281/zenodo.3931989
$Zγ$ production at NNLO including anomalous couplings
Creators: name: Campbell, John M.
name: Neumann, Tobias
name: Williams, Ciaran
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In this paper we present a next-to-next-to-leading order (NNLO) QCD calculation of the processes $pp\rightarrow l^+l^-γ$ and $pp\rightarrow ν\barνγ$ that we have implemented in MCFM. Our calculation includes QCD corrections at NNLO both for the Standard Model (SM) and additionally in the presence of $Zγγ$ and $ZZγ$ anomalous couplings. We compare our implementation, obtained using the jettiness slicing approach, with a previous SM calculation and find broad agreement. Focusing on the sensitivity of our results to the slicing parameter, we show that using our setup we are able to compute NNLO cross sections with numerical uncertainties of about $0.1\%$, which is small compared to residual scale uncertainties of a few percent. We study potential improvements using two different jettiness definitions and the inclusion of power corrections. At $\sqrt{s}=13$ TeV we present phenomenological results and consider $Zγ$ as a background to $H\to Zγ$ production. We find that, with typical cuts, the inclusion of NNLO corrections represents a small effect and loosens the extraction of limits on anomalous couplings by about $10\%$.
description: 30 pages, 14 figures
How Expanded Ionospheres of Hot Jupiters Can Prevent Escape of Radio Emission Generated by the Cyclotron Maser Instability
Creators: name: Weber, Christof
name: Lammer, Helmut
name: Shaikhislamov, Ildar
name: Chadney, Joshua
name: Khodachenko, Maxim
name: Grießmeier, Jean-Mathias
name: Rucker, Helmut
name: Vocks, Christian
name: Macher, Wolfgang
name: Odert, Petra
name: Kislyakova, Kristina
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present a study of plasma conditions in the atmospheres of the Hot Jupiters HD 209458b and HD 189733b and for an HD 209458b-like planet at orbit locations between 0.2-1 AU around a Sun-like star. We discuss how these conditions influence the radio emission we expect from their magnetospheres. We find that the environmental conditions are such that the cyclotron maser instability (CMI), the process responsible for the generation of radio waves at magnetic planets in the solar system, most likely will not operate at Hot Jupiters. Hydrodynamically expanding atmospheres possess extended ionospheres whose plasma densities within the magnetosphere are so large that the plasma frequency is much higher than the cyclotron frequency, which contradicts the condition for the production of radio emission and prevents the escape of radio waves from close-in exoplanets at distances <0.05 AU from a Sun-like host star. The upper atmosphere structure of gas giants around stars similar to the Sun changes between 0.2 and 0.5 AU from the hydrodynamic to a hydrostatic regime and this results in conditions similar to solar system planets with a region of depleted plasma between the exobase and the magnetopause where the plasma frequency can be lower than the cyclotron frequency. In such an environment, a beam of highly energetic electrons accelerated along the field lines towards the planet can produce radio emission. However, even if the CMI could operate the extended ionospheres of Hot Jupiters are too dense to let the radio emission escape from the planets.
Damping of quasi-2D internal wave attractors by rigid-wall friction
Creators: name: Beckebanze, F.
name: Brouzet, C.
name: Sibgatullin, I. N.
name: Maas, L. R. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The reflection of internal gravity waves at sloping boundaries leads to focusing or defocusing. In closed domains, focusing typically dominates and projects the wave energy onto 'wave attractors'. For small-amplitude internal waves, the projection of energy onto higher wave numbers by geometric focusing can be balanced by viscous dissipation at high wave numbers. Contrary to what was previously suggested, viscous dissipation in interior shear layers may not be sufficient to explain the experiments on wave attractors in the classical quasi-2D trapezoidal laboratory set-ups. Applying standard boundary layer theory, we provide an elaborate description of the viscous dissipation in the interior shear layer, as well as at the rigid boundaries. Our analysis shows that even if the thin lateral Stokes boundary layers consist of no more than 1% of the wall-to-wall distance, dissipation by lateral walls dominates at intermediate wave numbers. Our extended model for the spectrum of 3D wave attractors in equilibrium closes the gap between observations and theory by Hazewinkel et al. (2008).
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00064
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Archives Départementales De La Côte D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: comptes
subject: LaMOP

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00064, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
CONCENTRACIÓN DE METALES PESADOS EN BIVALVOS Anadara tuberculosa Y A. similis DEL ESTERO HUAYLÁ, PROVINCIA DE EL ORO, ECUADOR
Creators: name: Tobar, Johnny
name: Ramírez-Muñoz, Mery
name: Ivis Fermín
name: Senior, William
Publisher: name: figshare
Year: 2018
Subjects: subject: 40502 Chemical Oceanography
subject: FOS: Earth and related environmental sciences

description: Se determinan las concentraciones de metales pesados en los moluscos bivalvosAnadara similis y A. tuberculosa. Los ejemplares fueron recolectados a 2 km de ladesembocadura del Estero Huaylá, Provincia El Oro, Ecuador, en noviembre 2013.En el laboratorio se les determinaron la longitud y peso para cada una de las especies,estableciéndose dos intervalos de tallas para A. similis y cuatro para A. tuberculosa.La carne de los organismos fue extraída, lavada y secada en un horno a 60°C durante 72 h, para posteriormente digerirla con una mezcla de HNO3 y HClO4 enproporción 3:1. Las concentraciones de 4 metales: plomo, arsénico, mercurio y cadmio,fueron determinadas mediante espectrofotometría de absorción atómica. Losvalores promedio obtenidos en A. similis (mg/kg), fueron: Pb (8,51 ± 0,34); As (1,42± 0,06); Hg (618,7 \ pm 355,32); Cd (1,21 ± 0,23) mg / kg; mientras que A. tuberculosafueron: Pb (7,52 ± 0,46); As (1,55 ± 0,14); Hg (364,38 ± 91,39); Cd (1,68 ± 0,28) mg / kg.Las concentraciones registradas de Pb, As, Cd y Hg en ambas especies de moluscossuperan los límites máximos permisibles por las Normas Internacionales. Las tallasmás pequeñas (3-4 cm) de A. tuberculosa posee la capacidad de alcalde bioacumularcantidad de Pb, Hg y Cd, mientras que A. similis mostró su mayor concentración de Pb ensu talla más pequeña (4-5 cm).
Spectral semi-classical analysis of a complex Schrödinger operator in exterior domains
Creators: name: Almog, Yaniv
name: Grebenkov, Denis
name: Helffer, Bernard
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Generalizing previous results obtained for the spectrum of the Dirichlet and Neumann realizations in a bounded domain of a Schrödinger operator with a purely imaginary potential $h^2Δ+iV$ in the semiclassical limit $h\to 0$ we address the same problem in exterior domains. In particular we obtain the left margin of the spectrum, and the emptiness of the essential part of the spectrum under some additional assumptions.
Thalictrum dioicum Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Thalictrum
Thalictrum dioicum

description: Thalictrum dioicum, spec. nov.
5. Thalictrum floribus dioicis.
 Habitat in Canada . Kalm.
 Altitudo vix pedalis. Caulis rectus. Flores tetrapetali, corollis & staminibus 40 albis. Antherae flavescentes. 546 Foliola cernua sunt, qua nota distinctissima evadit planta ex habitu.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 545, DOI: 10.5281/zenodo.3931989
Supplementary material from Social network shrinking is explained by active and passive effects but not increasing selectivity with age in wild macaques
Creators: name: Sadoughi, Baptiste
name: Mundry, Roger
name: Schülke, Oliver
name: Ostner, Julia
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310499
subject: Evolutionary biology not elsewhere classified
classificationCode: 310901
subject: Animal behaviour

description: This file contains all supplementary methods, figures, and tables.
Thalictrum minus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Ranunculales
Ranunculaceae
Thalictrum
Thalictrum minus

description: Thalictrum minus, spec. nov.
6. Thalictrum foliis sexpartitis, floribus cernuis.
 Thalictrum caule folioso, foliolis caulinis acutis, panicula divaricata, floribus nutantibus. Fl. suec. 454. It. gotl. 180. * Dalib. paris. 454.
 Thalictrum minus. Bauh. pin. 337. Dod. pempt. 58.
 Ruta pratensis minor. Tabern. ic. 55.
 Habitat in Europae pratis. ♃
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 546, DOI: 10.5281/zenodo.3931989
Non-diagonal flavour observables in B and Collider Physics
Creators: name: Hurth, T.
name: Porod, W.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Until now the focus within the direct search for supersymmetry has mainly been on flavour diagonal observables. Recently lepton flavour violating signals at future electron positron colliders have been studied. There is now an opportunity to analyse the relations between collider observables and low-energy observables in the hadronic sector. In a first work in this direction, we study flavour violation in the squark decays of the second and third generations taking into account results from B physics, in particular from the rare decay b ->s gamma. Correlations between various squark decay modes can be used to get more precise information on various flavour violating parameters.
description: 3 pages, latex, Contribution to the International Europhysics Conference on High Energy Physics EPS03, 17-23 July 2003, Aachen, Germany
The NGC 454 system: anatomy of a mixed on-going merger
Creators: name: Plana, H.
name: Rampazzo, R.
name: Mazzei, P.
name: Marino, A.
name: Amram, Ph.
name: Ribeiro, A. L. B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This paper focuses on NGC 454, a nearby interacting pair of galaxies (AM0112-554, RR23), composed of an early-type (NGC 454 E) and a star forming late-type companion (NGC 454 W). We aim at characterizing this wet merger candidate via a multi-lambda analysis, from near-UV to optical using SWIFT-UVOT, and mapping the Halpha intensity (I) distribution, velocity (Vr), and velocity dispersion (sigma) fields with SAM+Perot-Fabry at SOAR observations. Luminosity profiles suggest that NGC 454 E is an S0. Distortions in its outskirts caused by the on-going interaction are visible in both optical and near-UV frames. In NGC 454 W, the NUV-UVOT images and the Halpha show a set of star forming complexes connected by a faint tail. Halpha emission is detected along the line connecting NGC 454 E to the NGC 454 main HII complex. We investigate the (I-sigma), (I-Vr ) (Vr-sigma) diagnostic diagrams of the HII complexes, most of which can be interpreted in a framework of expanding bubbles. In the main HII complex, enclosed in the UV brightest region, the gas velocity dispersion is highly supersonic reaching 60 km/s. However, Halpha emission profiles are mostly asymmetric indicating the presence of multiple components with an irregular kinematics. Observations point towards an advanced stage of the encounter. Our SPH simulations with chemophotometric implementation suggest that this mixed pair can be understood in terms of a 1:1 gas/halos encounter giving rise to a merger in about 0.2 Gyr from the present stage.
description: Accepted for publication in MNRAS (21pages, 20 figures)
Metales pesados (cadmio, plomo, mercurio) y arsénico en pescados congelados de elevado consumo en el Ecuador
Creators: name: Senior, William
name: Cornejo-Rodríguez, María Herminia
name: Tobar, Johnny
name: Ramírez-Muñoz, Mery R.
name: Márquez, Aristide
Publisher: name: figshare
Year: 2018
Subjects: subject: 40502 Chemical Oceanography
subject: FOS: Earth and related environmental sciences

description: Se realizó un estudio preliminar sobre el contenidode cadmio (Cd), plomo (Pb), mercurio (Hg) yarsénico (As) en muestras de peces de pescadocongelado de elevado consumo en El Ecuadorcomo, corvina (Cynoscion phoxocephalus), dorado(Coryphaena hippurus), tilapia (Oreochromis)niloticus) y atún (Thunnus obesus); adquiridos envarios supermercados de la ciudad de Machala,Provincia El Oro. Los resultados preliminaresmuestra la contaminación de estos productos porComo, Pb y Hg, superando las Normas Internacionalesestablecida para el consumo humano. En todaslas muestras examinadas los valores de Cdfueron inferiores al límite de detección del método(0,0042 mg. Kg-1). La correlación signifi cativa entreel contenido de Hg, Pb y como en las muestras demúsculo de pescado evaluadas, puede sugerirque son contaminantes tienen un origen comúnya que las elevadas concentraciones de As, Pb yHg hijo consecuencia de las aguas domésticas eindustriales vertidas sin tratamiento alguno en lazona costera así como, la escorrentía provenientede las zonas de cultivos y al frente atmosférico.
Machine Intelligence, New Interfaces, and the Art of the Soluble
Creators: name: Lyons, Michael J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences
subject: H.1.2; H.5.5

description: Position: (1) Partial solutions to machine intelligence can lead to systems which may be useful creating interesting and expressive musical works. (2) An appropriate general goal for this field is augmenting human expression. (3) The study of the aesthetics of human augmentation in musical performance is in its infancy.
description: CHI 2015 Workshop on Collaborating with Intelligent Machines: Interfaces for Creative Sound, April 18, 2015, Seoul, Republic of Korea
Note Illustrative della Carta geologica d'Italia alla scala 1:50.000, F. 299 Umbertide, Servizio Geologico d'Italia - ISPRA
Creators: name: Plesi, G.
Publisher: name: INFN Open Access Repository
Year: 2010

description: Note illustrative redatte per il Foglio geologico n. 299 Umbertide della Carta Geologica d'Italia alla scala 1:50.000. 299 pp.
A Keck/HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. I. Testing Giant Planet Formation and Migration Scenarios
Creators: name: Sozzetti, A.
name: Torres, G.
name: Latham, D. W.
name: Carney, B. W.
name: Stefanik, R. P.
name: Boss, A. P.
name: Laird, J. B.
name: Korzennik, S. G.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe a high-precision Doppler search for giant planets orbiting a well-defined sample of metal-poor dwarfs in the field. This experiment constitutes a fundamental test of theoretical predictions which will help discriminate between proposed giant planet formation and migration models. We present here details on the survey as well as an overall assessment of the quality of our measurements, making use of the results for the stars that show no significant velocity variation.
description: 25 pages, 7 figures, accepted for publication in the Astrophysical Journal