cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Rubus fruticosus Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rosaceae
Rubus
Rubus fruticosus

description: Rubus fruticosus Linnaeus, Species Plantarum 1: 493. 1753, typ. cons.
"Habitat in sepibus praesertim maritimis Europae." RCN: 3760.
Conserved type (van de Beek in Meded. Bot. Mus. Herb. Rijks Univ. Utrecht 415: 59. 1974; Weber in Bot. Jahrb. Syst. 106: 293, f. 1. 1986): Herb. Linn. No. 653.9, inflorescence only (LINN).
Generitype of Rubus Linnaeus, nom. cons.
Current name: Rubus fruticosus L. (Rosaceae).
Note: Rubus fruticosus, with the type designated by Weber, was proposed as conserved type of the genus by Jarvis (in Taxon 41: 573. 1992). This was eventually approved by the General Committee (see review of the history of this proposal by Barrie, l.c. 55: 795-796. 2006).
Rubus fruticosus has long been treated as an ambiguous name, and its type is identifiable with R. plicatus Weihe & Nees. Weber has provided a review, and restricted van de Beek’s (1974) type choice to the inflorescence only.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 801, DOI: 10.5281/zenodo.291971
Confirmation of double peaked Lyman-alpha emission at z=6.593: Witnessing a galaxy directly contributing to the reionisation of the Universe
Creators: name: Matthee, Jorryt
name: Sobral, David
name: Gronke, Max
name: Paulino-Afonso, Ana
name: Stefanon, Mauro
name: Röttgering, Huub
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Distant luminous Lyman-alpha emitters (LAEs) are excellent targets for spectroscopic observations of galaxies in the epoch of reionisation (EoR). We present deep high-resolution (R=5000) VLT/X-SHOOTER observations, along with an extensive collection of photometric data of `COLA1', a proposed double peaked LAE at z=6.6 (Hu et al. 2016). We rule out that COLA1's emission line is an [OII] doublet at z=1.475 on the basis of i) the asymmetric red line-profile and flux ratio of the peaks (blue/red=$0.31\pm0.03$) and ii) an unphysical [OII]/Ha ratio ([OII]/Ha > 22). We show that COLA1's observed B-band flux is explained by a faint extended foreground LAE, for which we detect Lya and [OIII] at z=2.142. We thus conclude that COLA1 is a real double-peaked LAE at z=6.593, the first discovered at z>6, confirming the result from Hu et al. (2016). COLA1 is UV luminous (M$_{1500}=-21.6\pm0.3$), has a high equivalent width (EW$_{0}$~120 Å) and very compact Lya emission (r$_{50} = 0.3$ kpc). Relatively weak inferred Hb+[OIII] line-emission from Spitzer/IRAC indicates an extremely low metallicity of Z<1/20 Z$_{\odot}$ or reduced strength of nebular lines due to high escape of ionising photons. The small Lya peak separation of $220\pm20$ km/s implies a low HI column density and an ionising photon escape fraction of ~15-30 %, providing the first direct evidence that such galaxies contribute actively to the reionisation of the Universe at z>6. Based on simple estimates, we find that COLA1 could have provided just enough photons to reionise its own ~0.3 pMpc bubble, allowing the blue Lya line to be observed. However, we also discuss alternative scenarios explaining the detected double peaked nature of COLA1. Our results show that future high-resolution observations of statistical samples of double peaked LAEs at z>5 are a promising probe of the occurrence of ionised regions around galaxies in the EoR.
description: 14 pages, 10 figures. Accepted for publication by A&A. Data are fully public
Reminiscences of William Wilson Cumberland, 1951
Publisher: name: Columbia University
Year: 2021
Subjects: Government consultants--United States
Economists
Economic history--20th century

description: Early life; research in Mexico on economic conditions, 1917; Paris Peace Conference with John Foster Dulles: economic decisions, personalities; economic adviser to State Department: post World War I economic conditions in United States and Europe; mandated territories; economies of Peru, Haiti, Nicaragua; stock market and United States economy; National Recovery Act, 1933; consultant, United Nations conference, 1945
Numerical Simulation of magnetized jet creation using a hollow ring of laser beams
Creators: name: Lu, Y.
name: Tzeferacos, P.
name: Liang, E.
name: Follett, R. K.
name: Gao, L.
name: Birkel, A.
name: Froula, D. H.
name: Fu, W.
name: Ji, H.
name: Lamb, D.
name: Li, C. K.
name: Sio, H.
name: Petrasso, R.
name: Wei, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Three dimensional FLASH magneto-hydrodynamics(MHD) modeling is carried out to interpret the OMEGA laser experiments of strongly magnetized, highly collimated jets driven by a ring of 20 OMEGA beams. The predicted optical Thomson scattering spectra and proton images are in good agreement with a subset of the experimental data. Magnetic fields generated via the Biermann battery term are amplified at the boundary between the core and the surrounding of the jet. The simulation predicts multiple axially aligned magnetic flux ropes with alternating poloidal component. Future applications of the hollow ring configuration in laboratory astrophysics are discussed.
On the Spectrum and Nature of the Peculiar Type Ia Supernova 1991T
Creators: name: Fisher, A.
name: Branch, D.
name: Hatano, K.
name: Baron, E.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A parameterized supernova synthetic-spectrum code is used to study line identifications in the photospheric-phase spectra of the peculiar Type Ia SN 1991T, and to extract some constraints on the composition structure of the ejected matter. The inferred composition structure is not like that of any hydrodynamical model for Type Ia supernovae. Evidence that SN 1991T was overluminous for an SN Ia is presented, and it is suggested that this peculiar event probably was a substantially super-Chandrasekhar explosion that resulted from the merger of two white dwarfs.
description: 1 text, 7 figures, submitted to MNRAS
Angiotensin (ang) 1-7 inhibits ang II-induced atrial fibrosis through regulating the interaction of proto-oncogene tyrosine-protein kinase Src (c-Src) and Src homology region 2 domain-containing phosphatase-1 (SHP-1))
Creators: name: Lu, Li
name: Cao, Li
name: Liu, Yihao
name: Chen, Yunlin
name: Fan, Jinqi
name: Yin, Yuehui
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: To verify whether Ang-(1-7) produces an antagonistic effect on Ang II-mediated atrial remodeling. Ang II–induced HL-1 cell model and a rat model of Ang II–induced atrial remodeling were constructed and intervened with Ang II Ang-(1-7), AngII +Ang-(1-7), Ang II+ c-Src specific inhibitor (SU6656), and Ang II + Ang-(1-7) + SSG (SHP-1/2 specific inhibitor, stibogluconate), respectively. The systolic blood pressure of the rat caudal artery was detected. And trial fibrosis was detected by Picrosirius red staining and Masson’s trichrome staining. Expressions of transforming growth factor-β (TGF-β), tissue inhibitor of metalloproteinases 1 (TIMP1), Matrix metalloproteinase 2 (MMP-2), connective tissue growth factor (CTGF), galectin-3, α-smooth muscle actin (α-SMA), and collagen I/III were subjected to qPCR and western blot. Furthermore, SHP-1 binding to c-Src was verified by co-immunoprecipitation (Co-IP). Results showed that the expressions of TGF-β, TIMP1, MMP-2, CTGF, α-SMA, galectin-3, and collagen I were increased markedly in the Ang II intervention group, and the expressions of p-ERK1/2, p-Akt, and p-p38MAPK were also increased dramatically. Ang-(1-7) or SU6656 addition could inhibit the action of Ang II factor, thereby minimizing the expressions of the previously described genes and proteins. Simultaneously, SSG supplement reversed the antagonistic effect of Ang-(1-7) on Ang II, and the latter elevated the blood pressure and induced atrial fibrosis in rats. Ang-(1-7) could reverse the changes related to Ang II–induced atrial fibrosis in rats. In conclusion, Ang-(1-7) antagonized Ang II–induced atrial remodeling by regulating SHP-1 and c-Src, thereby affecting the MAPKs/Akt signaling pathway.
Laser-to-droplet alignment sensitivity relevant for laser-produced plasma sources of extreme ultraviolet light
Creators: name: Reijers, Sten A.
name: Kurilovich, Dmitry
name: Torretti, Francesco
name: Gelderblom, Hanneke
name: Versolato, Oscar O.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: We present and experimentally validate a model describing the sensitivity of the tilt angle, expansion and propulsion velocity of a tin micro-droplet irradiated by a 1 μm Nd:YAG laser pulse to its relative alignment. This sensitivity is particularly relevant in industrial plasma sources of extreme ultraviolet light for nanolithographic applications. Our model has but a single parameter: the dimensionless ratio of the laser spot size to the effective size of the droplet, which is related to the position of the plasma critical density surface. Our model enables the development of straightforward scaling arguments in turn enabling precise control the alignment sensitivity.
description: 7 pages, 5 figures
Supplementary document for Ground-based high-resolution remote sensing of Sulphur hexafluoride (SF6) over Hefei, China: characterization, optical misalignment influence and variability - 5444264.pdf
Creators: name: Yin, Hao
name: SUN, YouWen
name: Wang, Wei
name: Shan, Changgong
name: Tian, Yuan
name: Liu, Cheng
Publisher: name: Optica Publishing Group
Year: 2021
Subjects: Uncategorized

description: The Haidinger fringes at the maximum OPD (the maximum misalignment position). The Haidinger fringes at 1/2 maximum OPD (the maximum misalignment position).
Synthesis and antitumor activity of benzophenone compound
Creators: name: Zhou, Bei-Dou
name: Wei, Rong-Rong
name: Li, Jia-Li
name: Yu, Zi-Han
name: Weng, Zhi-Min
name: Ruan, Zhi-Peng
name: Lin, Jian
name: Fang, Yuan-Yuan
name: Xu, Gui-Fen
name: Hu, Dong-Bao
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Information Systems not elsewhere classified

description: Seven benzophenone compounds were synthesized in one or two steps, then their antitumor activity was evaluated. The total yields ranged from 9% to 44%. Compounds 3c–5c exhibited obvious antitumor activity. Among them, compounds 3c and 4c exhibited excellent and broad-spectrum antitumor activity. Compound 3c exhibited much stronger inhibitory activities against fourteen cancer cells than cisplatin. In particular, compound 3c exhibited stronger cytotoxicity against hepatocarcinoma SMMC-7721 cells than Taxol, with a half maximal inhibitory concentration (IC50) of approximately 0.111 μM. These results demonstrated that compounds 3c, 4c and 5c were very promising antitumor leads for further structural modification.
Antiproliferative effect of secofriedelanophyllemblicine, a triterpenoid present in the roots of Phyllanthus emblica L
Creators: name: Wang, Cuifang
name: Xu, Huaimeng
name: Wang, Yixuan
Publisher: name: Taylor & Francis
Year: 2021
Subjects: Biochemistry
Cell Biology
Pharmacology
Biotechnology
Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Cancer
Hematology

description: Phyllanthus emblica L. is a widely distributed tropical medicinal plant with good therapeutic properties. In the present study, the chemical constituents isolation of the roots of P. emblica were carried out and six known compounds (1-6) were purified and their structures were determined by means of spectroscopic analysis. The known triterpenoid, secofriedelanophyllemblicine (1), was selected to check for its cytotoxic effect on a series of human tumor cells and normal cells. Secofriedelanophyllemblicine exhibited cell growth inhibition specifically on MCF-7 breast cancer cells when compared to other tested cell lines. Further flow cytometric analysis showed that secofriedelanophyllemblicine could inhibit cell proliferation and induced G2 phase arrest in the cell-cycle progression of MCF-7 cells. The gathered results suggest that secofriedelanophyllemblicine is a cell-cycle regulator in MCF-7 human breast cancer cells and might be used as a candidate chemopreventive agent for breast cancer prevention and intervention.
The absorption spectra of Q1107+487 and Q1442+295
Creators: name: Carballo, R.
name: Barcons, X.
name: Webb, J. K.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first moderate resolution (approx. 40--120 km/s) spectroscopic observations of the bright (V<16.7) high-redshift QSOs Q1107+487 (z_{em} = 2.965) and Q1442+295 (z_{em} = 2.669) (Sanduleak & Pesch 1989). The relatively high signal to noise reached in the spectra along with an extensive wavelength coverage of the Lyman alpha and the Lyman beta forest allowed us to obtain, through profile fitting, column densities and Doppler parameters of the Lyman clouds towards these QSOs. The spectral coverage of regions longward of the Lyman alpha emission line of the QSOs at the expected wavelengths of CIV 1548,1550 at the redshifts of the Lyman alpha forest allowed us to identify some heavy element absorption systems (hereafter HEASs) towards these QSOs. We have found no Lyman absorption system or HEAS towards these QSOs for which our data allow a deuterium measurement or to provide an interesting upper limit for the D/H ratio. The reason for this is that the Lyman lines with high column density detected towards these QSOs belong to absorption systems showing velocity structure.
description: Two postscript files (Text+1Figure) compressed and uuencoded. Proceedings of the ESO Workshop on QSO Absorption Lines. A more extensive work is accepted at AJ (April 1995 issue)
MOESM1 of Physiciansâ utilization of microbiologic reports and determinants of their preference to order culture in Tikur Anbessa Specialized Hospital, Addis Ababa, Ethiopia
Creators: name: Getachew Alemkere
name: Getu Gilagil
name: Teklu Gebrehiwot
name: Zelalem Tilahun
name: Hylemariam Mengist
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Additional file 1. Types of systemic bacterial infections suspected or proven in hospitalized patients in the internal medicine ward of TASH in 2014, Addis Ababa, Ethiopia.
Dark Matter and the Chemical Evolution of Irregular Galaxies
Creators: name: Carigi, L.
name: Colin, P.
name: Peimbert, M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present three types of chemical evolution models for irregular galaxies: closed-box with continuous star formation rates (SFRs), closed-box with bursting SFRs, and O-rich outflow with continuous SFRs. We discuss the chemical evolution of the irregular galaxies NGC 1560 and II Zw 33, and a ``typical'' irregular galaxy. The fraction of low-mass stars needed by our models is larger than that derived for the solar vicinity, but similar to that found in globular clusters. For our typical irregular galaxy we need a mass fraction of about 40% in the form of substellar objects plus non baryonic dark matter inside the Holmberg radius, in good agreement with the results derived for NGC 1560 and II Zw 33 where we do have an independent estimate of the mass fraction in non baryonic dark matter. Closed-box models are better than O-rich outflow models in explaining the C/O and Z/O observed values for our typical irregular galaxy.
description: 14 pages, 2 figure, uses emulateapj.sty package. ApJ in press. New models were added. The order of Tables has been corrected
Additional file 1: of Brain network alterations in individuals with and without mild cognitive impairment: parallel independent component analysis of AV1451 and AV45 positron emission tomography
Creators: name: Li, Yuan
name: Yao, Zhijun
name: Yu, Yue
name: Zou, Ying
name: Fu, Yu
name: Hu, Bin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified

description: Acquisition parameters of PET data. We have revised in the manuscript. (DOCX 13 kb)
High Resolution Mid-Infrared Imaging of the Nucleus of NGC 1068
Creators: name: Bock, J. J.
name: Marsh, K. A.
name: Ressler, M. E.
name: Werner, M. W.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained mid-infrared images of the nucleus of NGC 1068 from the Hale 5 m telescope at Mt. Palomar with diffraction-limited resolution and high sensitivity at 8.8, 10.3, and 12.5 microns. Deconvolved images show that the infrared emission extends north to south in the inner 2", consisting of a central peak, a component extending 1" north of the central source, a component extending 1" south of the central source, and several smaller structures located 1" to the northeast. The central peak is extended 0.4" N-S and unresolved (<= 0.2") E-W. We find that 50 +/- 5% of the flux emerges from the central 0.4" and that a single unresolved point source can account for only 27 +/- 5% of the total flux. However, if the central peak arises from optically thick emission, we estimate that the emitting region has a projected area >= 2 pc^2, and may thus contain a compact source such as a parsec-scale torus. We observe a correspondence between the northern extension and the northeastern sources appearing on the mid-infrared images and the [OIII] clouds A-C & E. We interpret the faint optical counterpart to the mid-infrared southern extension as being due to partial obscuration by the intervening disk of the host galaxy. The N-S extension of the mid-infrared emission coincides with one wall of the conical narrow line region and aligns with the N-S orientation of the radio jet close to the nucleus. We interpret the infrared emission as arising from optically thick dust lining the walls of the low density cavity formed by the radio jet and heated by radiation from the central source.
description: accepted by Astrophysical Journal 29 June 1998, 18 pages, 2 figures
Additional file 1: of Evaluating the safety and feasibility of a new surgical treatment for forearm fractures in older children: study protocol for a randomised controlled trial
Creators: name: Chen, Chunhui
name: Xie, Linzhen
name: Zheng, Wenhao
name: Chen, Hua
name: Cai, Leyi
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Biotechnology
Cancer
Science Policy

description: SPIRIT 2013 checklist: recommended items to address in a clinical trial protocol and related documents. (DOC 124 kb)
B-spline ADC: many-body ab initio theory for electron dynamics in strong laser fields
Creators: name: Ruberti, Marco
Publisher: name: Imperial College London
Year: 2015

description: This thesis is focused on the development of an eﬃcient ﬁrst-principles theoretical and numerical method based on the many-electron algebraic diagrammatic construction [ADC(n)] schemes, in order to describe the correlated ionisation dynamics in atomic and molecular systems interacting with perturbative and non-perturbative laser ﬁelds. The ﬁrst line of research has focused on the calculation of total singlephoton photoionisation cross-sections, applying the Stieltjes-Imaging theory to Lanczos pseudospectra of the ADC Hamiltonian in Gaussian basis. We have established the accuracy of this technique by comparing the ADCLanczos-Stieltjes ground-state cross-sections obtained using diﬀerent levels of many-body theory to the experimental ones for a series of organic molecules. We have extended this method to excited states cross-sections showing that a theoretical modelling of photoionisation from excited states requires an intrinsically double excitation theory. However, above 80 eV photon energy all three methods lead to inaccurate results due to the limitations of the Gaussian basis to describe continuum wave-functions of ionised electrons. The second, main line of research, has therefore been dedicated to constructing and computationally optimising the ﬁrst implementation of the single [ADC(1)] and double excitations [ADC(2)] schemes in the B-spline basis, which is able to accurately describe the strongly oscillating continuum orbitals. As ﬁrst application of this new method, we have calculated the photoionisation cross-sections of noble gas atoms showing that the features that pose a challenge for the GTO calculations are reproduced in a very good agreement with the experiment. We also have developed a time-dependent version with which we have calculated the HHG spectra of Ar, reproducing the eﬀect of the Cooper minimum, and CO2, quantitatively investigating the multi-channel eﬀects on its dynamical minimum. Finally we have provided a numerical answer to the highly topical question of coherence and ionic wavepacket formation in short pulse photoionisation.
Additional file 2: of An open-source tool to identify active travel from hip-worn accelerometer, GPS and GIS data
Creators: name: Procter, Duncan
name: Page, Angie
name: Cooper, Ashley
name: Nightingale, Claire
name: Ram, Bina
name: Rudnicka, Alicja
name: Whincup, Peter
name: Clary, Christelle
name: Lewis, Daniel
name: Cummins, Steven
name: Ellaway, Anne
name: Giles-Corti, Billie
name: Cook, Derek
name: Owen, Christopher
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Model accuracy for each cross-validation subset (DOCX 26Â kb)
Rubus hispidus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rosaceae
Rubus
Rubus hispidus

description: Rubus hispidus, spec. nov.
3. Rubus foliis ternatis nudis, caulibus petiolisque hispidis.
 Habitat in Canada . Kalm. ♄
 Caules viticulis longis, procumbentibus, lignosis, una cum petiolis adspersi setis rigidis. Folia ternata, nuda, inciso-serrata: intermedio pedicellato; pedunculi etjam hispidi.
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 493, DOI: 10.5281/zenodo.3931989
Rubus hispidus Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rosaceae
Rubus
Rubus hispidus

description: Rubus hispidus Linnaeus, Species Plantarum 1: 493. 1753.
"Habitat in Canada. Kalm." RCN: 3756.
Lectotype (Bailey in Gentes Herb. 1: 249. 1925): Kalm, Herb. Linn. No. 653.4 (LINN).
Current name: Rubus hispidus L. (Rosaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 801, DOI: 10.5281/zenodo.291971
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0200
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0200, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0200, 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
Additive perfect codes in Doob graphs
Creators: name: Shi, Minjia
name: Huang, Daitao
name: Krotov, Denis S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences
subject: 94B05, 94B25, 05B40

description: The Doob graph $D(m,n)$ is the Cartesian product of $m>0$ copies of the Shrikhande graph and $n$ copies of the complete graph of order $4$. Naturally, $D(m,n)$ can be represented as a Cayley graph on the additive group $(Z_4^2)^m \times (Z_2^2)^{n'} \times Z_4^{n''}$, where $n'+n''=n$. A set of vertices of $D(m,n)$ is called an additive code if it forms a subgroup of this group. We construct a $3$-parameter class of additive perfect codes in Doob graphs and show that the known necessary conditions of the existence of additive $1$-perfect codes in $D(m,n'+n'')$ are sufficient. Additionally, two quasi-cyclic additive $1$-perfect codes are constructed in $D(155,0+31)$ and $D(2667,0+127)$.
Molecular Gas in the Inner 3.2 Kiloparsecs of NGC 2403: Star Formation at Subcritical Gas Surface Densities
Creators: name: Thornley, Michele D.
name: Wilson, Christine D.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a fully sampled map of the inner 3.2 kpc of the nearby spiral galaxy NGC 2403 in the CO J=1-0 line. These data emphasize the relatively small contribution of molecular hydrogen to the cold gas content of this galaxy, and confirm that the gas surface densities in the inner 2.8 kpc of NGC 2403 lie below the critical surface density for star formation under the theory proposed by Kennicutt (1989). Since star formation is occurring throughout the inner disk, the simple dynamical model used by Kennicutt cannot be the only important process regulating star formation in galaxies. We suggest that stochastic star formation processes are responsible for the star formation seen in these regions, and thus that supercritical gas densities may not be a necessary condition for star formation in the inner regions of galactic disks.
description: 10 pages, plus 4 tables, 4 figures, and references; file is compressed, uuencoded Postscript. This paper has been accepted for publication in the 10 July 1995 issue of The Astrophysical Journal
Determinations of form factors for semileptonic $D\rightarrow K$ decays and leptoquark constraints
Creators: name: Zhang, Jian
name: Yue, Chong-Xing
name: Li, Chun-Hua
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: By analyzing all existing measurements for $ D\rightarrow K \ell^+ ν_{\ell} $ ( $\ell=e,\ μ$ ) decays, we find that the determinations of both the vector form factor $f_+^K(q^2)$ and scalar form factor $f_0^K(q^2)$ for semileptonic $D\rightarrow K$ decays from these measurements are feasible. By taking the parameterization of the one order series expansion of the $f_+^K(q^2)$ and $f_0^K(q^2)$, $f_+^K(0)|V_{cs}|$ is determined to be $0.7182\pm0.0029$, and the shape parameters of $f_+^K(q^2)$ and $f_0^K(q^2)$ are $r_{+1}=-2.16\pm0.007$ and $r_{01}=0.89\pm3.27$, respectively. Combining with the average $f_+^K(0)$ of $N_f=2+1$ and $N_f=2+1+1$ lattice calculaltion, the $|V_{cs}|$ is extracted to be $0.964\pm0.004\pm0.019$ where the first error is experimental and the second theoretical. Alternatively, the $f_+^K(0)$ is extracted to be $0.7377\pm0.003\pm0.000$ by taking the $|V_{cs}|$ as the value from the global fit with the unitarity constraint of the CKM matrix. Moreover, using the obtained form factors by $N_f=2+1+1$ lattice QCD, we re-analyze these measurements in the context of new physics. Constraints on scalar leptoquarks are obtained for different final states of semileptonic $D \rightarrow K$ decays.
Sensitivity Analysis of Cascaded Quantum Feedback Amplifier
Creators: name: Yokotera, Yu
name: Yamamoto, Naoki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum amplifier is an essential device in quantum information processing. As in the classical (non-quantum) case, its characteristic uncertainty needs to be suppressed by feedback, and in fact such a control theory for a single quantum amplifier has recently been developed. This letter extends this result to the case of cascaded quantum amplifier. In particular, we consider two types of structures: the case where controlled amplifiers are connected in series, and the case where a single feedback control is applied to the cascaded amplifier. Then, we prove that the latter is better in the sense of sensitivity to the uncertainty. A detailed numerical simulation is given to show actual performance of these two feedback schemes.
description: 6 pages, 6 figures, 1 table
Additional file 1: of An open-source tool to identify active travel from hip-worn accelerometer, GPS and GIS data
Creators: name: Procter, Duncan
name: Page, Angie
name: Cooper, Ashley
name: Nightingale, Claire
name: Ram, Bina
name: Rudnicka, Alicja
name: Whincup, Peter
name: Clary, Christelle
name: Lewis, Daniel
name: Cummins, Steven
name: Ellaway, Anne
name: Giles-Corti, Billie
name: Cook, Derek
name: Owen, Christopher
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: Characteristics of the training data and remainder of the cohort from ENABLE, for further detail and demographics see the baseline cohort paper (Ram et al., 2016, BMJ Open 6: e012643) (DOCX 15Â kb)
The observable 21cm signal from reionization may be perturbative
Creators: name: McQuinn, Matthew
name: D'Aloisio, Anson
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: We develop an effective perturbation theory (and, equivalently, a bias expansion) for the inhomogeneous 21cm radiation field from reionization. Using large-scale simulations of cosmological reionization, we find that this expansion describes the modes in the simulated 21cm signal over much of the wavenumber range probed by upcoming 21cm arrays. This result provides an understanding of the potential signal shapes that compliments the nonlinear numerical modeling that has been the focus of most previous work. We find that the observable signal often can be described with 2-3 bias coefficients that can be interpreted in terms of the source biases, the average neutral fraction, the characteristic size of ionized regions, and the patchiness of reionization. The 21cm signal serves as a wacky example of a bias expansion in cosmology, with our approach synthesizing key results.
description: 26 JCAP pages, 8 Figures; published in JCAP
Additional file 6: of A family of auxin conjugate hydrolases from Solanum lycopersicum and analysis of their roles in flower pedicel abscission
Creators: name: Fu, Xin
name: Shi, Zihang
name: Jiang, Yun
name: Jiang, Lingling
name: Qi, Mingfang
name: Xu, Tao
name: Li, Tianlai
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Hematology
subject: Plant Biology
subject: Virology

description: Primer for qRT-PCR and fusion protein. (DOC 29 kb)
Poly(vinylidene fluoride) membranes
Creators: name: Ji, Jing
Publisher: name: Imperial College London
Year: 2016

description: Poly(vinylidene fluoride) (PVDF) membranes have been intensively investigated and commercialised with broad applications in water purification and wastewater treatment for decades due to its outstanding properties. Currently, PVDF membranes are mainly produced by the phase inversion technique, which is predominant in both laboratory research and industrial manufacturing. Various modification methods based on the phase inversion technique have also been developed to improve the membrane performances, but these improvements are incremental and there have been no important breakthroughs during the past decade. This thesis first explores the preparation of reinforced PVDF flat sheet membranes by blending nanoclay followed by the phase inversion process. Although the membranes showed improved water permeation flux and enhanced abrasion resistance, further improvements are limited by the phase inversion technique itself. Consequently, a new concept of membrane manufacturing procedure has been proposed by combining unidirectional crystallisation of green solvent and polymer diffusion. The new method uses crystallites of a solvent dimethyl sulfoxide with controlled sizes as pore templates to create enormous nanosized flow passages. It follows a completely different pore formation mechanism and therefore overcomes the drawbacks of the phase inversion technique. The resultant PVDF membranes have an asymmetric structure composed of a highly porous separation layer and gradually opened micro-channels. Due to the unique structure, the prepared membranes showed excellent permeation performances and mechanical properties overwhelming commercial PVDF membranes prepared by the phase inversion technique. The filtration performance of the PVDF membranes can be further improved by modification of the membrane material, for example, by blending polyethylene glycol in the dope solution. The obtained membrane with pore size of 36 nm showed extraordinary high flux of 1711 L/m2h and could withstand 35 bar in the test. Moreover, the new manufacturing process is of much fewer influencing factors compared to the phase inversion approach and thus highly reliable and repeatable. In principle, it is also applicable to other common polymeric membrane materials such as polyethersulfone and cellulose acetate.
Rubus idaeus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rosaceae
Rubus
Rubus idaeus

description: Rubus idaeus, spec. nov.
 1. Rubus foliis quinato-pinnatis ternatisque, caule 493 aculeato, petiolis canaliculatis. Fl. suec. 408. Mat. med. 242.
 Rubus caule erecto hispido, foliis ternatis. Fl. lapp. 204. Hort. cliff. 192. Hort. ups. 133. Roy. lugdb. 273.
 Rubus idaeus spinosus. Bauh. pin. 479.
 β. Rubus idaeus fructu albo. Bauh. pin. 479.
 γ. Rubus idaeus laevis. Bauh. pin. 479.
 Habitat in Europae lapidosis. ♃ ♂
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 492-493, DOI: 10.5281/zenodo.3931989
A computational mechanistic investigation of calcium catalysed hydrophosphination
Creators: name: Ward, Bryan James
Publisher: name: Imperial College London
Year: 2015

description: The calcium-catalysed intermolecular hydrophosphination reaction is an atom efficient synthetic route to organophosphines. Early experimental studies indicated a correspondence between the hydroamination and hydrophosphination reactions. However, we recognise a need for a theoretical investigation of the intermolecular hydrophosphination reaction particularly as many aspects of the mechanism remain poorly understood. The work within this thesis describes a theoretical investigation of the intermolecular hydrophosphination reaction catalysed by the [beta]-diketiminate stabilised Ca complex, [{HC(C(Me)N-2,6-iPr2C6H3)2}Ca{PPh2}(THF)]. Preliminary DFT calculations were performed on a simplified model of the experimental system. The intermolecular hydrophosphination of ethene is a stepwise mechanism involving alkene insertion and protonolysis, consistent with experimental results. Calculations demonstrate the importance of secondary stabilising interactions, particularly the Ca–[pi] interaction, which coordinates preferentially over a Ca–P interaction. Calculations involving the substitution of ethene for styrene and vinylpyridine were also performed (Chapter 4). Stabilisation of the alkylphosphine fragment through the arene ring allowed for considerably more interchange between important secondary bonding interactions. During the styrene hydrophosphination reaction the kinetically most favourable protonolysis pathway proceeded from an alkylphosphine fragment that exhibited no secondary stabilising interaction. Such a coordination mode has not been considered previously in previous hydroamination reaction studies. Calculations were also performed to investigate the hydrophosphination reaction mechanism for an experimentally representative catalyst (Chapter 5). A ligand-based proton-assisted mechanism was identified involving a multi-centre transition state. In the ligand-based mechanism the alkylphosphine product was generated alongside the active catalyst in a single step. The single step, ligand-based mechanism was a kinetically more favourable pathway and thermodynamically representative of experiment. To the best of the author’s knowledge, this is the first example of the Ae catalysed heterofunctionalisation reaction, which demonstrates preference for a ligand-based mechanism.
Rubus idaeus Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Rosaceae
Rubus
Rubus idaeus

description: Rubus idaeus Linnaeus, Species Plantarum 1: 492. 1753.
"Habitat in Europae lapidosis." RCN: 3754.
Lectotype (Chater & al. in Edees & Newton, Brambles Brit. Isles: 18. 1988): Herb. Linn. No. 653.1 (LINN).
Current name: Rubus idaeus L. (Rosaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 801, DOI: 10.5281/zenodo.291971
Approximate input physics for stellar modelling
Creators: name: Pols, O. R.
name: Tout, C. A.
name: Eggleton, P. P.
name: Han, Z.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a simple and efficient, yet reasonably accurate, equation of state, which at the moderately low temperatures and high densities found in the interiors of stars less massive than the Sun is substantially more accurate than its predecessor by Eggleton, Faulkner & Flannery. Along with the most recently available values in tabular form of opacities, neutrino loss rates, and nuclear reaction rates for a selection of the most important reactions, this provides a convenient package of input physics for stellar modelling. We briefly discuss a few results obtained with the updated stellar evolution code.
description: uuencoded compressed postscript. The preprint are also available at http://www.ast.cam.ac.uk/preprint/PrePrint.html
Reminiscences of William and Marguerite Zorach, 1957
Publisher: name: Columbia University
Year: 2021
Subjects: Painters
Sculptors
Sculpture, Modern--20th century
Painting, Modern--20th century

description: Early life in Cleveland; study at the National Academy and in Europe; return to New York and first work in stone; commissioned monuments; citizenship difficulties; plate-by-plate discussion of Paul Wingert's THE SCULPTURE OF WILLIAM ZORACH; work habits; artistic philosophy
Dust Spirals and Acoustic Noise in the Nucleus of the Galaxy NGC 2207
Creators: name: Elmegreen, B. G.
name: Elmegreen, D. M.
name: Brinks, E.
name: Yuan, C.
name: Kaufman, M.
name: Klaric, M.
name: Montenegro, L.
name: Struck, C.
name: Thomasson, M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations with the Hubble Space Telescope reveal an irregular network of dust spiral arms in the nuclear region of the interacting disk galaxy NGC 2207. The spirals extend from ~50 pc to ~300 pc in galactocentric radius, with a projected width of ~20 pc. Radiative transfer calculations determine the gas properties of the spirals and the inner disk, and imply a factor of ~4 local gas compression in the spirals. The gas is not strongly self-gravitating, nor is there a nuclear bar, so the spirals could not have formed by the usual mechanisms applied to main galaxy disks. Instead, they may result from acoustic instabilities that amplify at small galactic radii. Such instabilities may promote gas accretion into the nucleus.
description: 4 pages, two figures, accepted by Astrophysical J. Letters, Vol 503, August 20, 1998
Role of thin organic interlayers inserted at the electrode interfaces for efficient polymer LEDs
Creators: name: Bailey, Jim
Publisher: name: Imperial College London
Year: 2014

description: This thesis discusses role of thin organic interlayers at the electrode interfaces of polymer light-emitting diodes (LEDs) in increasing their efficiencies. The effect of varying the anode-side IL material, its thickness, and its p-doping level on poly(dioctylfluorene-alt-benzothiadiazole) (F8BT) PLEDs is examined. Then the impact of varying the IL material is explored in Lumation Green 1300 PLEDs to determine whether a relation exists between the role of the IL and the light emitting layer's properties. It is found that excitons are formed in F8BT adjacent to the interface with the IL and are thus exceptionally sensitive to the energetics at that interface, with wide energy gaps helping to reduce luminance quenching significantly. The general effects of ionic cathode-side ILs on PLED efficiencies and response times are investigated. The novel materials used contain imidazolium cationic groups. The impact of varying the ionic IL main conjugated backbone on PLED characteristics is studied, since the conjugated backbone is primarily responsible for the optoelectronic properties of semiconducting polymers. Efficiencies of ~15 lm W-1 at 3 V are achieved. The light emitting layer is varied from F8BT to Super Yellow to probe the influence of the active layer's properties on the role of the IL in determining device characteristics. The exact combination of active layer and IL strongly influence device performance. The influence of the mobile anion and the immobile cationic group of cathode-side ILs on PLED performance is investigated. Our investigation focused on ionic ILs with a F8BT conjugated backbone. Ionic ILs with various mobile counter ions are created to study the role of the mobile ion on charge injection. Increased size of anion leads to poorer device performances. Experiments were carried out to understand what factors determine the response times and efficiencies of PLEDs with ionic cathode-side ILs. Response times of 4.24 μs are recorded and Scanning Kelvin Probe Microscopy (SKPM) experiments on thin films of the ionic polymers are conducted to shed light on the movement of ions within the IL during PLED operation. Good energy level matching with the cathode metal is found for the ionic cathode-side ILs, allowing for good electron injection properties.
The Nuclear Impact on Cosmology: The $H_0\hbox{-}Ω$ Diagram
Creators: name: Copi, Craig J.
name: Schramm, David N.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The \HOmega\ diagram is resurrected to dramatically illustrate the nature of the key problems in physical cosmology today and the role that nuclear physics plays in many of them. In particular it is noted that the constraints on \OmegaB\ from big bang nucleosynthesis do not overlap with the constraints on \OmegaVis\ nor have significant overlap with the lower bound on $Ω$ from cluster studies. The former implies that the bulk of the baryons are dark and the later is the principle argument for non-baryonic dark matter. A comparison with hot x-ray emitting gas in clusters is also made. The lower bound on the age of the universe from globular cluster ages (hydrogen burning in low mass stars) and from nucleocosmochronology also illustrates the Hubble constant requirement $H_0 \le 66 \Hunits$ for $Ω_0 = 1$\@. It is also noted that high values of $H_0$ ($\sim 80\Hunits$) even more strongly require the presence of non-baryonic dark matter. The lower limit on $H_0$ ($\ge 38\Hunits$) from carbon detonation driven type~Ia supernova constrains long ages and only marginally allows \OmegaB\ to overlap with \OmegaClus. Diagrams of \HOmega\ for $Λ_0=0$ and $Λ_0\neq 0$ are presented to show that the need for non-baryonic dark matter is independent of $Λ$.
description: 10 pages, LaTeX(2.09), 4 figures. A nicely formatted postscript version of the text with encapsulated figures can be found at ftp://astro.uchicago.edu/pub/astro/HOmega (see the README file for details)