cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Corinnomma Karsch 1880
Creators: name: Raven, Robert J.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Corinnidae
Corinnomma

description: Corinnomma Karsch, 1880
Corinnomma Karsch, 1880: 374, type species by original designation Corinna severa Thorell, 1877: 481; Deeleman-Reinhold, 2001: 316
Diagnosis. Corinnomma differs from Castoponera by the gradually sloping anterior abdomen (Fig. 12a, rather than the overhanging edge) and from Poecilipta in the dorsal scute being fused to the ventral scute (Fig. 13e) and in the cylindrical palpal tibia without ventral concavity (Fig. 13b).
Distribution. Presently known from south-east Asia and Africa but the African species seems misplaced.
Remarks. Although all species of Asian Corinnomma treated by Deeleman-Reinhold (2001), except for C. thorelli Simon, 1905, have a paracymbial spine, the significance of the character in Corinnomma is not clear. Certainly, in some Australian genera, the paracymbial spine can be present or absent.
Misplaced Species. Haddad (2006) noted that, unlike the Asian species, African species of Corinnomma have a slightly recurved posterior eye row, and as here noted, lack a paracymbial spine. Hence, Corinnomma olivaceum Simon, 1896, Corinnomma semiglabrum (Simon, 1896) and Corinnomma lawrencei Haddad, 2006 are considered misplaced in the genus.
description: Published as part of Raven, Robert J., 2015, & lt; strong & gt; A revision of ant-mimicking spiders of the family Corinnidae (Araneae) in the Western Pacific & lt; / strong & gt;, pp. 1-258 in Zootaxa 3958 (1) on page 31, DOI: 10.11646/zootaxa.3958.1.1, http://zenodo.org/record/14951911
Smyrnium connatum Boiss. & Kotschy
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
Apiales
Apiaceae
Smyrnium
Smyrnium connatum

description: Smyrnium aegyptiacum Linnaeus, Centuria I Plantarum: 10. 1755.
"Habitat in Aegypto. D. Hasselquist." RCN: 2094.
Type not designated.
Original material: Herb. Linn. No. 370.2 (LINN).
 Current name:  Smyrnium connatum  Boiss. & Kotschy (Apiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 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 859, DOI: 10.5281/zenodo.291971
Initial States: IR and Collinear Divergences
Creators: name: Lavelle, Martin
name: McMullan, David
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The standard approach to the infra-red problem is to use the Bloch-Nordsieck trick to handle soft divergences and the Lee-Nauenberg (LN) theorem for collinear singularities. We show that this is inconsistent in the presence of massless initial particles. Furthermore, we show that using the LN theorem with such initial states introduces a non-convergent infinite series of diagrams at any fixed order in perturbation theory.
description: 4 pages, talk given at Montpellier meeting QCD'06 (to appear in the proceedings)
Comment on "Relation between scattering amplitude and Bethe-Salpeter wave function in quantum field theory"
Creators: name: Aoki, Sinya
name: Doi, Takumi
name: Hatsuda, Tetsuo
name: Ishii, Noriyoshi
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We invalidate the arguments given in [T.Yamazaki and Y.Kuramashi, Phys. Rev. D96, 114511 (2017)] over the HAL QCD method for hadron-hadron interactions on the lattice. We also pose questions on the practical usefulness of the method proposed in this reference.
description: 3 pages. Version accepted for publication in Physical Review D
Impact of $θ_{13}$ on Lepton Flavour Violating processes within SUSY Seesaw
Creators: name: Antusch, S.
name: Arganda, E.
name: Herrero, M. J.
name: Teixeira, A. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the impact of neutrino masses and mixings on LFV processes within the context of the supersymmetric seesaw scenario, where the CMSSM is extended by three right-handed (s)neutrinos. A hierarchical spectrum is considered for both heavy and light neutrinos. We systematically analyse the interesting relation between the leptonic mixing angle $θ_{13}$ and LFV muon and tau decays, namely $l_j \to l_i γ$ and $l_j \to 3 l_i$, and discuss the interplay with the other relevant parameters. We require compatibility with low energy neutrino data, bounds on both LFV decays and charged lepton electric dipole moments, and impose a successful baryogenesis via thermal leptogenesis. Particular emphasis is given to the implications that a future $θ_{13}$ measurement can have on our knowledge of the heavy neutrino sector.
description: 44 pages, 25 figures. Some comments and references added. Version to appear in JHEP
Finite Size Scaling in 2d Causal Set Quantum Gravity
Creators: name: Glaser, Lisa
name: O'Connor, Denjoe
name: Surya, Sumati
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the $N$-dependent behaviour of $\mathrm{2d}$ causal set quantum gravity. This theory is known to exhibit a phase transition as the analytic continuation parameter $β$, akin to an inverse temperature, is varied. Using a scaling analysis we find that the asymptotic regime is reached at relatively small values of $N$. Focussing on the $\mathrm{2d}$ causal set action $S$, we find that $β\langle S\rangle $ scales like $ N^ν$ where the scaling exponent $ν$ takes different values on either side of the phase transition. For $β> β_c$ we find that $ν=2$ which is consistent with our analytic predictions for a non-continuum phase in the large $β$ regime. For $β
description: 32 pages, 27 figures (v2 typos and missing reference fixed)
The Redshift Completeness of Local Galaxy Catalogs
Creators: name: Kulkarni, S. R.
name: Perley, D. A.
name: Miller, A. A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: There is considerable interest in understanding the demographics of galaxies within the local universe (defined, for our purposes, as the volume within a radius of 200 Mpc or z<0.05). In this pilot paper, using supernovae (SNe) as signposts to galaxies, we investigate the redshift completeness of catalogs of nearby galaxies. In particular, type Ia SNe are bright and are good tracers of the bulk of the galaxy population, since they arise in both old and young stellar populations. Our input sample consists of SNe with redshift < 0.05, discovered by the flux-limited ASAS-SN survey. We define the redshift completeness fraction (RCF) as the number of SN host galaxies with known redshift prior to SN discovery, determined, in this case, via the NASA Extragalactic Database (NED), divided by the total number of newly discovered SNe. Using SNe Ia, we find RCF = 78 (+6, -7, 90% confidence interval) for z < 0.03. We examine the distribution of host galaxies with and without cataloged redshifts as a function of absolute magnitude and redshift, and, unsurprisingly, find that higher-z and fainter hosts are less likely to have a known redshift prior to the detection of the SN. However, surprisingly, some L* galaxies are also missing. We conclude with thoughts on the future improvement of RCF measurements that will be made possible from large SN samples resulting from ongoing and especially upcoming time-domain surveys.
description: Submitted to ApJ
Zizia aurea W. D. J. Koch 1824
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
Apiales
Apiaceae
Zizia
Zizia aurea

description: Smyrnium aureum Linnaeus, Species Plantarum 1: 262. 1753.
"Habitat in America boreali." RCN: 2096.
 Lectotype (Reveal & al. in Huntia 7: 236. 1987): Herb. Linn. No. 370.5 (LINN).
 Current name:  Zizia aurea  (L.) W.D.J. Koch (Apiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 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 859, DOI: 10.5281/zenodo.291971
The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses
Creators: name: Pessah, Martin E.
name: Chan, Chi-kwan
name: Psaltis, Dimitrios
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Numerical simulations of turbulent, magnetized, differentially rotating flows driven by the magnetorotational instability are often used to calculate the effective values of alpha viscosity that is invoked in analytical models of accretion discs. In this paper we use various dynamical models of turbulent magnetohydrodynamic stresses, as well as numerical simulations of shearing boxes, to show that angular momentum transport in MRI-driven accretion discs cannot be described by the standard model for shear viscosity. In particular, we demonstrate that turbulent magnetorotational stresses are not linearly proportional to the local shear and vanish identically for angular velocity profiles that increase outwards.
description: Updated to match published version in MNRAS, 8 pages, 1 figure
Corinnomma severum
Creators: name: Raven, Robert J.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Corinnidae
Corinnomma
Corinnomma severum

description: Corinnomma severum (Thorell, 1877)
(Fig. 12a–d)
Corinna severum Thorell, 1877: 481.
Corinnomma severum: Karsch, 1880: 374. For full synonymy, see Deeleman-Reinhold, 2001: 318.
Material. Indonesia: 1♂, Sumatra Median, Dollok, MNHNP 24197, det. as Corinnomma by E. Simon.
Diagnosis. Males differ from those of C. javanum in the screw-like embolus tip (see Deeleman-Reinhold, 2001, fig. 469) and females in the relatively larger, closely spaced CO.
Supplementary description. Male palp with socketed sessile paracymbial spine, tibia cylindrical with slightly raised distal edge. Male and female: femora III, IV without distal constriction; three pairs of long spines on ventral tibiae I and II, two similar pairs on metatarsi I, II; distinct but light scopula for metatarsi and tarsi I, II. Carapace of female with fine pustules, larger in males. Females with small (anterior one-sixth) dorsal scute but no ventral scute; no paragenital brackets; chelicerae with low fang shield and 8–9 long curved serrate bristles; retrolateral face of chelicerae smooth. Male with dorsal scute for full length and wraps around abdomen to ventral edge and slopes gradually to anterior edge; laterally fused to genital scute and covering book lungs; distinct ventral scute (Fig. 12a). Carapace profile long and flat with steep anterior and posterior edges; female and to lesser extent male with Vshaped depression anterior to fovea. Pedicel without collar. Tracheal scute broad, curved at edges in male and female.
Remarks. Deeleman-Reinhold, 2001: fig. 465 shows a full scute indicative that the type is a male (according to the description and my observations) but the caption states it is the female.
description: Published as part of Raven, Robert J., 2015, & lt; strong & gt; A revision of ant-mimicking spiders of the family Corinnidae (Araneae) in the Western Pacific & lt; / strong & gt;, pp. 1-258 in Zootaxa 3958 (1) on page 32, DOI: 10.11646/zootaxa.3958.1.1, http://zenodo.org/record/14951911
Central exclusive production of longlived gluinos at the LHC
Creators: name: Bussey, P. J.
name: Coughlin, T. D.
name: Forshaw, J. R.
name: Pilkington, A. D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We examine the possibility of producing gluino pairs at the LHC via the exclusive reaction pp -> p+gluino+gluino+p in the case where the gluinos are long lived. Such long lived gluinos are possible if the scalar super-partners have large enough masses. We show that it may be possible to observe the gluinos via their conversion to R-hadron jets and measure their mass to better than 1% accuracy for masses below 350 GeV with 300/fb of data.
description: 13 pages, 9 figures. Minor corrections to version 1
Additional file 3: of Oxidative stress enhances tumorigenicity and stem-like features via the activation of the Wnt/Î˛-catenin/MYC/Sox2 axis in ALK-positive anaplastic large-cell lymphoma
Creators: name: Chengsheng Wu
name: Gupta, Nidhi
name: Yung-Hsing Huang
name: Zhang, Hai-Feng
name: Abdulraheem Alshareef
name: Chow, Alexandra
name: Lai, Raymond
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Figure S3. The serial dilution experiment in RU and RR cells derived from Karpas 299 cells. The serial diluted RU and RR cells derived from Karpas 299 (from 1000 cells to 1 cell) were seeded in 96-well plates. After 8Â days, the number of spheres was counted in the highlighted wells circulated by the rectangle lines. The right panel showed the analyzed results which indicated that converted RR cells and native RR cells with H2O2 stimulation have formed more spheres in a lower number of cells seeded (125 cells for RU cells and converted RR cells, 32 cells for RR cells and RR cells with H2O2 stimulation), as compared with native RU and RR cells, respectively. Note that RR cells also have formed more spheres than RU cells at a lower number of cells seeded (i.e. 32 and 63 cells). (PDF 259 kb)
Wooden Shoes for a Favourite Niece
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: At the end of the war, my great uncle Pete Marceau was billeted with a family in the Netherlands after spending six long years fighting overseas. They discovered he had a beloved niece Mary Lou (my mother) back home in Canada and crafted a pair of wooden shoes for him to send to her. Despite having almost no food themselves, they still managed to stuff the shoes with candy for the little girl. This act of generosity and appreciation still chokes me up to this day. A few years ago, my mother gave the wooden shoes to my daughter Holly with a letter describing them as part of her heritage.
Directed clustering in weighted networks: a new perspective
Creators: name: Clemente, Gian Paolo
name: Grassi, Rosanna
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Social and Information Networks (cs.SI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: In this paper, we consider the problem of assessing local clustering in complex networks. Various definitions for this measure have been proposed for the cases of networks having weighted edges, but less attention has been paid to both weighted and directed networks. We provide a new local clustering coefficient for this kind of networks, starting from those existing in the literature for the weighted and undirected case. Furthermore, we extract from our coefficient four specific components, in order to separately consider different link patterns of triangles. Empirical applications on several real networks from different frameworks and with different order are provided. The performance of our coefficient is also compared with that of existing coefficients in the literature.
Radiative transfer simulations of cosmic reionization I: methodology and initial results
Creators: name: Trac, Hy
name: Cen, Renyue
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new hybrid code for large volume, high resolution simulations of cosmic reionization, which utilizes a N-body algorithm for dark matter, physically motivated prescriptions for baryons and star formation, and an adaptive ray tracing algorithm for radiative transfer of ionizing photons. Two test simulations each with 3 billion particles and 400 million rays in a 50 Mpc/h box have been run to give initial results. Halos are resolved down to virial temperatures of 10^4 K for the redshift range of interest in order to robustly model star formation and clumping factors. This is essential to correctly account for ionization and recombination processes. We find that the halos and sources are strongly biased with respect to the underlying dark matter, re-enforcing the requirement of large simulation boxes to minimize cosmic variance and to obtain a qualitatively correct picture of reionization. We model the stellar initial mass function (IMF), by following the spatially dependent gas metallicity evolution, and distinguish between the first generation, Population III (PopIII) stars and the second generation, Population II (PopII) stars. The PopIII stars with a top-heavy IMF produce an order of magnitude more ionizing photons at high redshifts z>10, resulting in a more extended reionization. In our simulations, complete overlap of HII regions occurrs at z~6.5 and the computed mass and volume weighted residual HI fractions at 5
description: 15 pages, 13 figures; accepted by ApJ; higher resolution figures can be found at http://www.astro.princeton.edu/~htrac/reionization.html
Achieving higher standards in species distribution modeling by leveraging the diversity of available software: tutorials
Creators: name: Kass, Jamie M.
name: Smith, Adam B.
name: Warren, Dan L.
name: Vignali, Sergio
name: Aiello-Lammens, Matthew E.
name: Arlé, Eduardo
name: Barbosa, Ana Marcia
name: Broennimann, Olivier
name: Cobos, Marlon E.
name: Guéguen, Maya
name: Osorio-Olvera, Luis
name: Owens, Hannah L.
name: Pinilla Buitrago, Gonzalo
name: Sánchez-Tapia, Andrea
name: Schmitt, Sylvain
name: Valavi, Roozbeh
name: Velazco, Santiago José Elías
name: Zizka, Alexander
name: Zurell, Damaris
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 310402
subject: Biogeography and phylogeography
classificationCode: 460207
subject: Modelling and simulation

description: There are many tools for species distribution modeling in R, so many in fact that sorting through them and deciding which to use for what can be an overwhelming exercise. This repository provides pdf files of the three supplemental vignettes (i.e., tutorials) described in Kass et al. (2024) that highlight how pluralistic use of R package tools can enhance analyses. All vignettes present full SDM analyses from data collection and processing to model building and predictions, and two of them provide walkthroughs for shiny applications. This first release (1.0.0) is planned to be updated over time to adapt to new package versions.
Photos of William Percival Edens (1907-1980)
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: See attached photos of William Percival Edens (1907-1980)
A comparison between the detection of gamma rays and positrons from neutralino annihilation
Creators: name: Mambrini, Y.
name: Munoz, C.
name: Nezri, E.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the indirect detection of neutralino dark matter using positrons and gamma rays from its annihilation in the galactic halo. Considering the HESS data as the spectrum constituting the gamma--ray background, we compare the prospects for the experiments GLAST and PAMELA in a general supergravity framework with non--universal scalar and gaugino masses. We show that with a boost factor of about 10, PAMELA will be competitive with GLAST for typical NFW cuspy profiles.
description: 18 pages, 6 figures, 1 reference added. Final version to appear in JCAP
Taenidia integerrima Drude 1898
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
Apiales
Apiaceae
Taenidia
Taenidia integerrima

description: Smyrnium integerrimum Linnaeus, Species Plantarum 1: 263. 1753.
"Habitat in Virginia." RCN: 2097.
 Lectotype (Reveal in Jarvis & al. in Taxon 55: 215. 2006): Clayton 549, Herb. Linn. No. 370.7 (LINN; iso- BM).
 Current name:  Taenidia integerrima  (L.) Drude (Apiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 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 859, DOI: 10.5281/zenodo.291971
The mass function of GX 339-4 from spectroscopic observations of its donor star
Creators: name: Heida, M.
name: Jonker, P. G.
name: Torres, M. A. P.
name: Chiavassa, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We obtained 16 VLT/X-shooter observations of GX 339-4 in quiescence in the period May - September 2016 and detected absorption lines from the donor star in its NIR spectrum. This allows us to measure the radial velocity curve and projected rotational velocity of the donor for the first time. We confirm the 1.76 day orbital period and we find that $K_2$ = $219 \pm 3$ km s$^{-1}$, $γ= 26 \pm 2$ km s$^{-1}$ and $v \sin i = 64 \pm 8$ km s$^{-1}$. From these values we compute a mass function $f(M) =1.91 \pm 0.08~M_{\odot}$, a factor $\sim 3$ lower than previously reported, and a mass ratio $q = 0.18 \pm 0.05$. We confirm the donor is a K-type star and estimate that it contributes $\sim 45-50\%$ of the light in the $J$- and H-band. We constrain the binary inclination to $37^\circ < i < 78^\circ$ and the black hole mass to $2.3~M_{\odot} < M_\mathrm{BH} < 9.5~M_{\odot}$. GX 339-4 may therefore be the first black hole to fall in the 'mass-gap' of $2-5~M_{\odot}$.
description: 11 pages, 7 figures, accepted for publication in ApJ
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 026
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: LaMOP
subject: Chartes de la Bourgogne du Moyen Âge
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 026, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 026, 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
Melanesotypus Raven, 2015, gen. nov.
Creators: name: Raven, Robert J.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Corinnidae
Melanesotypus

description: Melanesotypus gen. nov.
Diagnosis. Males differ from those of Apochinomma Pavesi, 1881 in the presence of a paracymbial spine (Fig. 15b–d) and from those of Sphecotypus in lacking a well-developed mentum and a subquadrate anterior sternal projection, Bonaldo, in litt.). Carapace strongly constricted medially dorsoventrally (Fig. 14e, f); back eye row much wider than front row and clearly recurved (Fig. 15a); male palpal bulb simple (Fig. 15b), as in most castianeirines.
Description. See description of M. guadal sp. nov.
Type Species: Melanesotypus guadal sp. nov.
Etymology. The generic name derives from the Melanesian islands.
description: Published as part of Raven, Robert J., 2015, & lt; strong & gt; A revision of ant-mimicking spiders of the family Corinnidae (Araneae) in the Western Pacific & lt; / strong & gt;, pp. 1-258 in Zootaxa 3958 (1) on page 35, DOI: 10.11646/zootaxa.3958.1.1, http://zenodo.org/record/14951911
Revision of VLT/UVES constraints on a varying fine-structure constant
Creators: name: Murphy, Michael T.
name: Webb, John K.
name: Flambaum, Victor V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We critically review the current null results on a varying fine-structure constant, alpha, derived from VLT/UVES quasar absorption spectra, focusing primarily on the many-multiplet analysis of 23 absorbers from which Chand et al. (2004) reported a weighted mean relative variation of da/a=(-0.06+/-0.06) x 10^{-5}. Our analysis of the same reduced data, using the same fits to the absorption profiles, yields very different individual da/a values with uncertainties typically larger by a factor of ~3. We attribute the discrepancies to flawed parameter estimation techniques in the original analysis and demonstrate that the original da/a values were strongly biased towards zero. Were those flaws not present, the input data and spectra should have given a weighted mean of da/a=(-0.44+/-0.16) x 10^{-5}. Although this new value does reflect the input spectra and fits (unchanged from the original work -- only our analysis is different), we do not claim that it supports previous Keck/HIRES evidence for a varying alpha: there remains significant scatter in the individual da/a values which may stem from the overly simplistic profile fits in the original work. Allowing for such additional, unknown random errors by increasing the uncertainties on da/a to match the scatter provides a more conservative weighted mean, da/a=(-0.64+/-0.36) x 10^{-5}. We highlight similar problems in other current UVES constraints on varying alpha and argue that comparison with previous Keck/HIRES results is premature.
description: 11 pages, 7 figures (10 EPS files). Accepted by MNRAS. v3: Added figure summarizing all current UVES constraints; added references and corrected typos
Grandmother's 1945 Recipe for Christmas Pudding
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: Marjorie Clarke moved out of London with her son and daughter to escape bombing and ran a pub in a place called Compton Chamberlain in Wiltshire during the war. Her grandson thinks they got the recipe from a wartime cookbook and originally it had powdered eggs.4oz self raising flour
4oz breadcrumbs
4oz finely chopped suet or other fat
half level teaspoonful of ground cinnamon
half level teaspoonful of salt
half level teaspoonful of grated nutmeg
half level teaspoonful of mixed spice
14 oz of mixed dried fruit
1oz blanched chopped almonds or other nuts or alternatively almond flavouring
3oz sugar, preferably brown
2 level tablespoonfuls tepid golden syrup
1 tablespoonful of marmalade
2 shell eggs or reconstituted dried eggs
about three quarters gill of stout
This pudding can be made right away or at any convenient time before Christmas. If margarine, or other fat is used instead of suet melt it. Pick over and dry clean fruit, stone and quarter raisins. Chop peel in marmalade. Warm syrup before measuring. Sift together into a mixing bowl the flour, salt and spices, add breadcrumbs, fruit, including nuts, if being used, sugar, suet or melted fat, mixing well after each addition. Stir beaten eggs with tepid syrup, stir in marmalade, also almond flavouring if nuts are omitted. Stir the liquid into dry ingredients and add enough stout to make a mixture of the usual dropping consistency. Stir well to mix thoroughly. Put into a greased basin, 2 pint size, tie down with a double thickness of greased grease-proof paper, steam for 6 hours. When cold remove paper, tie down with clean paper and a cloth, store in a cool, airy place, preferably hung up. When wanted steam for two and a half hours.Our family are still making this pudding and I always use suet. For the fruit I use just sultanas and the brown sugar. Do not use Guinness for the stout as it is too bitter.
Neutrinos and Ultra-High-Energy Cosmic-Ray Nuclei from Blazars
Creators: name: Rodrigues, Xavier
name: Fedynitch, Anatoli
name: Gao, Shan
name: Boncioli, Denise
name: Winter, Walter
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We discuss the production of ultra-high-energy cosmic ray (UHECR) nuclei and neutrinos from blazars. We compute the nuclear cascade in the jet for both BL Lac objects and flat-spectrum radio quasars (FSRQs), and in the ambient radiation zones for FSRQs as well. By modeling representative spectral energy distributions along the blazar sequence, two distinct regimes are identified, which we call "nuclear survival" -- typically found in low-luminosity BL Lacs, and "nuclear cascade" -- typically found in high-luminosity FSRQs. We quantify how the neutrino and cosmic-ray (CR) emission efficiencies evolve over the blazar sequence, and demonstrate that neutrinos and CRs come from very different object classes. For example, high-frequency peaked BL Lacs (HBLs) tend to produce CRs, and HL-FSRQs are the more efficient neutrino emitters. This conclusion does not depend on the CR escape mechanism, for which we discuss two alternatives (diffusive and advective escape). Finally, the neutrino spectrum from blazars is shown to significantly depend on the injection composition into the jet, especially in the nuclear cascade case: Injection compositions heavier than protons lead to reduced neutrino production at the peak, which moves at the same time to lower energies. Thus, these sources will exhibit better compatibility with the observed IceCube and UHECR data.
description: 23 pages, 20 figures
Additional file 8 of CircMRPS35 suppresses gastric cancer progression via recruiting KAT7 to govern histone modification
Creators: name: Jie, Mengmeng
name: Wu, Yaran
name: Gao, Mengyuan
name: Li, Xinzhe
name: Liu, Cheng
name: Ouyang, Qin
name: Tang, Qingyun
name: Shan, Changyu
name: Lv, Yangfan
name: Zhang, Kebin
name: Dai, Qian
name: Chen, Yang
name: Zeng, Shuo
name: Li, Chenglin
name: Wang, Liting
name: He, Fengtian
name: Hu, Changjiang
name: Yang, Shiming
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 8: Figure S3. Restoration of FOXO1 and FOXO3a Partially Reversed CircMRPS35-Induced Suppression of Gastric Cancer Progression. Related to Fig. 5. Figure S4. Molecular Docking of the Interactions of CircMRPS35/KAT7/H4K5ac and the Design of ChIP Primers. Related to Fig. 7
Smyrnium olusatrum 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
Apiales
Apiaceae
Smyrnium
Smyrnium olusatrum

description: Smyrnium olusatrum Linnaeus, Species Plantarum 1: 262. 1753.
"Habitat in Scotia, Wallia, Gallia." RCN: 2095.
 Lectotype (Jafri in Jafri & El-Gadi, Fl. Libya 117: 32. 1985): Herb. Clifford: 105, Smyrnium 2 (BM-000558366).
 Generitype of Smyrnium Linnaeus (vide Hitchcock, Prop. Brit. Bot.: 141. 1929).
 Current name:  Smyrnium olusatrum  L. (Apiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 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 859, DOI: 10.5281/zenodo.291971
title: 03_0619
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Poem about Evacuation from Dunkirk
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: Although he did type letters to his family during the war, it is unknown if he was the author. This typed up poem is amongst the war papers and photos from Lt. Col. A.W. Shirley, who served with the Ox. and Bucks. at Dunkirk and throughout the Second World War. Although he did type letters to his family during the war, it is unknown if he was the author. He was evacuated from Dunkirk. He had previously served in the First World War also.
MOESM3 of Considerations for expanding community exercise programs incorporating a healthcare-recreation partnership for people with balance and mobility limitations: a mixed methods evaluation
Creators: name: Salbach, Nancy
name: Jo-Anne Howe
name: Baldry, Diem
name: Saira Merali
name: Munce, Sarah
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Computational Biology

description: Additional file 3. TIMETM Survey Questionnaire.
Effects of non-standard neutrino-electron interactions on relic neutrino decoupling
Creators: name: Mangano, Gianpiero
name: Miele, Gennaro
name: Pastor, Sergio
name: Pinto, Teguayco
name: Pisanti, Ofelia
name: Serpico, Pasquale D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider the decoupling of neutrinos in the early Universe in presence of non-standard neutral current neutrino-electron interactions (NSI). We first discuss a semi-analytical approach to solve the relevant kinetic equations and then present the results of fully numerical and momentum-dependent calculations, including flavor neutrino oscillations. We present our results in terms of both the effective number of neutrino species (N_eff) and the impact on the abundance of He-4 produced during Big Bang Nucleosynthesis. We find that, for NSI parameters within the ranges allowed by present laboratory data, non-standard neutrino-electron interactions do not essentially modify the density of relic neutrinos nor the bounds on neutrino properties from cosmological observables, such as their mass. Nonetheless, the presence of neutrino-electron NSI may enhance the entropy transfer from electron-positron pairs into neutrinos instead of photons, up to a value of N_eff=3.12. This is almost three times the correction to N_eff=3 that appears for standard weak interactions.
description: 23 pages, 5 figures. To be published in NPB
The Impact of Environment on the Stellar Mass - Halo Mass Relation
Creators: name: Golden-Marx, Jesse B.
name: Miller, Christopher J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A large variance exists in the amplitude of the Stellar Mass - Halo Mass (SMHM) relation for group and cluster-size halos. Using a sample of 254 clusters, we show that the magnitude gap between the brightest central galaxy (BCG) and its second or fourth brightest neighbor accounts for a significant portion of this variance. We find that at fixed halo mass, galaxy clusters with a higher magnitude gap have a higher BCG stellar mass. This relationship is also observed in semi-analytic representations of low-redshift galaxy clusters in simulations. This SMHM-magnitude gap stratification likely results from BCG growth via hierarchical mergers and may link assembly of the halo with the growth of the BCG. Using a Bayesian model, we quantify the importance of the magnitude gap in the SMHM relation using a multiplicative stretch factor, which we find to be significantly non-zero. The inclusion of the magnitude gap in the SMHM relation results in a large reduction in the inferred intrinsic scatter in the BCG stellar mass at fixed halo mass. We discuss the ramifications of this result in the context of galaxy formation models of centrals in group and cluster-sized halos.
description: 17 pages, 17 figures, accepted for publication in ApJ
title: V2_DU_LettreN
Creators: name: Basnage de Beauval, Henri
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Ceci est la V2 du Dictionnaire universel, revu et corrigé en 1701 par Basnage de Beauval. Cette version a été obtenue avec GROBID dictionaries, après adaptation du système et renentraînement en juillet 2020.
Rotating metric in Non-Singular Infinite Derivative Theories of Gravity
Creators: name: Cornell, Alan S.
name: Harmsen, Gerhard
name: Lambiase, Gaetano
name: Mazumdar, Anupam
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we will provide a non-singular rotating space time metric for a ghost free infinite derivative theory of gravity. We will provide the predictions for the Lense-Thirring effect for a slowly rotating system, and how it is compared with that from general relativity.
description: 5 pages; Accepted for publishing in PRD
Smyrnium perfoliatum 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
Apiales
Apiaceae
Smyrnium
Smyrnium perfoliatum

description: Smyrnium perfoliatum Linnaeus, Species Plantarum 1: 262. 1753.
"Habitat in Italia, Creta." RCN: 2093.
 Lectotype (Turland & Reduron in Jarvis & al. in Taxon 55: 215. 2006): Herb. Linn. No. 370.1 (LINN).
 Current name:  Smyrnium perfoliatum  L. (Apiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 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 859, DOI: 10.5281/zenodo.291971
SN 2006gy: An extremely luminous supernova in the galaxy NGC 1260
Creators: name: Ofek, E. O.
name: Cameron, P. B.
name: Kasliwal, M. M.
name: Gal-Yam, A.
name: Rau, A.
name: Kulkarni, S. R.
name: Frail, D. A.
name: Chandra, P.
name: Cenko, S. B.
name: Soderberg, A. M.
name: Immler, S.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With an extinction-corrected V-band peak absolute magnitude of about -22, supernova (SN) 2006gy is probably the brightest SN ever observed. We report on multi-wavelength observations of this SN and its environment. Our spectroscopy shows an H alpha emission line as well as absorption features which may be identified as SiII lines at low expansion velocity. The high peak luminosity, the slow rise to maximum, and the narrow H alpha line are similar to those observed in hybrid type-Ia/IIn (also called IIa) SNe. The host galaxy, NGC 1260, is dominated by an old stellar population with solar metallicity. However, our high resolution adaptive optics images reveal a dust lane in this galaxy, and there appears to be an HII region in the vicinity of the SN. The extra-ordinarily large peak luminosity, ~3x10^44 erg/s, demands a dense circum-stellar medium, regardless of the mass of the progenitor star. The inferred mass loss rate of the progenitor is ~0.1 solar mass per year over a period of ~10 yr prior to explosion. Such an high mass-loss rate may be the result of a binary star common envelope ejection. The total radiated energy in the first two months is about 1.1x10^51 erg, which is only a factor of two less than that available from a super-Chandrasekhar Ia explosion. Therefore, given the presence of a star forming region in the vicinity of the SN and the high energy requirements, a plausible scenario is that SN 2006gy is related to the death of a massive star (e.g., pair production SN).
description: 4 pages, ApJL, submitted
The Strong CP Problem and Axions
Creators: name: Peccei, R. D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I describe how the QCD vacuum structure, necessary to resolve the $U(1)_A$ problem, predicts the presence of a P, T and CP violating term proportional to the vacuum angle $\barθ$. To agree with experimental bounds, however, this parameter must be very small $(\barθ \leq 10^{-9}$). After briefly discussing some possible other solutions to this, so-called, strong CP problem, I concentrate on the chiral solution proposed by Peccei and Quinn which has associated with it a light pseudoscalar particle, the axion. I discuss in detail the properties and dynamics of axions, focusing particularly on invisible axion models where axions are very light, very weakly coupled and very long-lived. Astrophysical and cosmological bounds on invisible axions are also briefly touched upon.
description: 14 pages, to appear in the Lecture Notes in Physics volume on Axions, (Springer Verlag)
Pte Horwell in Belgium
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: Pte Horwell was called up in March 1942, aged 37. His record of service shows he was with the West Yorks for four months then transferred to the Lancashire Fusilliers for 10 months. He joined the Corps of Military Police, perhaps unsurprising given his age, from May 1943 to May 1946. He was with 73 Coy CMP when the photograph was taken, I think, in Belgium. I have a company photograph of him in front of the Brabo fountain in Antwerp and know he ended his time overseas in Hannover in 1946 but have not otherwise been able to fill in a timeline for his movements/locations.