cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000775
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: registre
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Châtelet

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1000775
Delphinium cuneatum Steven ex DC.
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
Ranunculales
Ranunculaceae
Delphinium
Delphinium cuneatum

description: Delphinium × hybridum Linnaeus, Demonstr. Pl Horto Upsaliensi: 15. 1753.
RCN: 3951.
Type not designated.
Original material: Herb. Linn. No. 218.19 (S); Herb. Linn. No. 694.9 (LINN).
 Current name:  Delphinium cuneatum  Steven ex DC. (Ranunculaceae).
 Note: Burtt (in Kew Bull. 9: 68. 1954) stated "The true D. hybridum, of which there is a specimen in the Linnean herbarium, is the same as D. cuneatum Stev. ". Subsequently, Chowdhuri & al. (in Notes Roy. Bot. Gard. Edinburgh 22: 404. 1958) stated that "the specimen in the Linnaean herbarium...must be accepted as the type", but did not distinguish between 694.9 and 694.10 (LINN). They rejected the name as a nomen confusum. It does not appear to be in use and should probably be a candidate for formal rejection.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 477, DOI: 10.5281/zenodo.291971
Transient and Sharvin resistances of Luttinger liquids
Creators: name: Kloss, Thomas
name: Weston, Joseph
name: Waintal, Xavier
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Although the intrinsic conductance of an interacting one-dimensional system is renormalized by the electron-electron correlations, it has been known for some time that this renormalization is washed out by the presence of the (non-interacting) electrodes to which the wire is connected. Here, we study the transient conductance of such a wire: a finite voltage bias is suddenly applied across the wire and we measure the current before it has enough time to reach its stationary value. These calculations allow us to extract the Sharvin (contact) resistance of Luttinger and Fermi liquids. In particular, we find that a perfect junction between a Fermi liquid electrode and a Luttinger liquid electrode is characterized by a contact resistance that consists of half the quantum of conductance in series with half the intrinsic resistance of an infinite Luttinger liquid. These results were obtained using two different methods: a dynamical Hartree-Fock approach and a self-consistent Boltzmann approach. Although these methods are formally approximate we find a perfect match with the exact results of Luttinger/Fermi liquid theory.
description: 6 pages, 3 figures, final version
Continuous statistics of the Lyman-alpha forest at 0 < z < 1.6: the mean flux, flux distribution, and autocorrelation from HST FOS spectra
Creators: name: Kirkman, David
name: Tytler, David
name: Lubin, Dan
name: Charlton, Jane
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We measure the amount of absorption in the Lyman-alpha forest at 0 < z < 1.6 in HST FOS spectra of 74 QSOs. At 0 < z < 1.6 we find that 79% of the absorption is from the low density intergalactic medium, 12% from metals and 9% from the strong H I lines, nearly identical to the percentages (78, 15 and 7) that we measured independently at z=2 from spectra taken with the Kast spectrograph on the Lick 3-m. At z=1 the low density intergalactic medium absorbs 0.037 +/- 0.004 of the flux. The error includes some but not all of the uncertainty in the continuum level. The remaining part gives relative errors of approximately 0.21 when we report the mean absorption in eight independent redshift intervals, and 0.047 when we average over all redshifts. We find 1.46 times more absorption from the low density intergalactic medium than comes from Ly-alpha lines that Bechtold et al. 2002 listed in the same spectra. The amount of absorption increases with z and can be fit by a power law in (1+z) with index 1.01. This corresponds to no change in the number of lines, of fixed rest frame equivalent widths, per unit redshift, consistent with the Janknecht et al. 2006 results on the distribution of lines. When we include similar measurements from higher redshifts, we need more degrees of freedom to fit the amount of absorption at 0 < z < 3.2. A power law with a break in slope, changing from index 1.5 at low z to 3.0 above z ~ 1.1 is a better but only marginally acceptable fit. We also calculate two other continuous statistics, the flux probability distribution function and the flux autocorrelation function that is non zero out to v ~ 500 km/sec at 0.5 < z < 1.5.
description: 12 pages, submitted to MNRAS
Radiative corrections to hard spectator scattering in $B\to ππ$ decays
Creators: name: Kivel, Nikolai
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the calculation of the next-to-leading corrections to the tree amplitudes which appear in the description of non-leptonic B-decays in the factorization approach. These corrections, together with radiative corrections to the jet functions, represent the full next-to-leading contributions to the dominant hard spectator scattering term generated by operators $O_{1,2}$ in the decay amplitudes. Using obtained analytical results we estimate $B\toππ$ branchings fractions in the physical (or BBNS) factorization scheme. We have also found that the imaginary part generated in the hard spectator scattering term is rather large compared to the imaginary part of the vertex contribution.
description: text is improved and typos are corrected, accepted for publication in JHEP
Additional file 12: of Unexpected conservation of the RNA splicing apparatus in the highly streamlined genome of Galdieria sulphuraria
Creators: name: Qiu, Huan
name: Rossoni, Alessandro W.
name: Weber, Andreas
name: Yoon, Hwan
name: Debashish Bhattacharya
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S6. Estimation of gains and losses of conserved introns in red algal phylogeny. (PDF 92Â kb)
Survivors of the Sunken "King John", 1940
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: Please note that this submission contains links to websites that are created and maintained by other individuals and organisations. The viewpoints expressed on those websites do not necessarily represent the views of the Their Finest Hour project team or the University of Oxford. In July 1940 my Grandfather, Ralph Richardson from Goathland, North Yorkshire was a marine engineer on board the British Merchant Navy ship the King John. Whilst it sailed in the South Atlantic his ship was attacked and eventually sunk by the German auxiliary cruiser the Widder. Prior to the ships sinking the crew abandoned ship into the lifeboats and were allowed by the Widder's Captain to drift and find land as best they could. After several days at sea, they fortunately managed to make land at St Kitts in the West Indies. My Grandmother who heard of the King John's sinking was naturally very upset since she didn't know whether my Grandfather was alive or dead for six months.He survived and continued his career as a marine engineer working for Listers. He died in 1963 and he was buried at St Mary's church in Goathland.I would have very much enjoyed asking him questions about his wartime experiences but I was only five years old when he died.Please see below links to further information about the King John and how the crew survived the sinking plus details of the German raider 'Widder':https://www.bandcstaffregister.com/page4551.html
https://en.wikipedia.org/wiki/German_auxiliary_cruiser_widder
Quantum information transmission through a qubit chain with quasi-local dissipation
Creators: name: Radgohar, Roya
name: Memarzadeh, Laleh
name: Mancini, Stefano
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study quantum information transmission in a Heisenberg-XY chain where qubits are affected by quasi-local environment action and compare it with the case of local action of the environment. We find that for open boundary conditions the former situation always improves quantum state transfer process, especially for short chains. In contrast, for closed boundary conditions quasi-local environment results advantageous in the strong noise regime. When the noise strength is comparable with the XY interaction strength, the state transfer fidelity through chain of odd/even number of qubits in presence of quasi-local environment results smaller/greater than that in presence of local environment.
Longitude-resolved imaging of Jupiter at lambda = 2 cm
Creators: name: Sault, R. J.
name: Engel, C.
name: de Pater, Imke
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a technique for creating a longitude-resolved image of Jupiter's thermal radio emission. The technique has been applied to VLA data taken on 25 January 1996 at a wavelength of 2 cm. A comparison with infrared data shows a good correlation between radio hot spots and the 5 micron hot spots seen on IRTF images. The brightest spot on the radio image is most likely the hot spot through which the Galileo probe entered Jupiter's atmosphere. We derived the ammonia abundance (= volume mixing ratio) in the hot spot, which is ~ 3 x 10^{-5}, about half that seen in longitude-averaged images of the NEB, or less than 1/3 of the longitude-averaged ammonia abundance in the EZ. This low ammonia abundance probably extends down to at least the 4 bar level.
Convolutional Dictionary Learning: A Comparative Review and New Algorithms
Creators: name: Garcia-Cardona, Cristina
name: Wohlberg, Brendt
Publisher: name: arXiv
Year: 2017
Subjects: subject: Machine Learning (cs.LG)
subject: Image and Video Processing (eess.IV)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Convolutional sparse representations are a form of sparse representation with a dictionary that has a structure that is equivalent to convolution with a set of linear filters. While effective algorithms have recently been developed for the convolutional sparse coding problem, the corresponding dictionary learning problem is substantially more challenging. Furthermore, although a number of different approaches have been proposed, the absence of thorough comparisons between them makes it difficult to determine which of them represents the current state of the art. The present work both addresses this deficiency and proposes some new approaches that outperform existing ones in certain contexts. A thorough set of performance comparisons indicates a very wide range of performance differences among the existing and proposed methods, and clearly identifies those that are the most effective.
description: Corrected typos in Eq. (18) and (19)
Hypothalamic expression analysis of m6A RNA methylation associated genes suggests a potential role of epitransciptomics in sexual maturation of Atlantic salmon
Creators: name: Ahi, Ehsan Pashay
name: Frapin, Morgane
name: Hukkanen, Mikaela
name: Primmer, Craig R.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Genomics (q-bio.GN)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: Better understanding the molecular processes contributing to variation in maturation timing is important for Atlantic salmon aquaculture, as early maturation causes considerable financial losses. The m6A RNA methylation is a conserved and dynamically reversible mechanism controlling gene expression in a myriad of biological processes. The role of m6A methylation in sexual maturation, however, has remained largely unexplored and has never been studied in Atlantic salmon. While the maturation process is known to be affected by many genetic and environmental factors, the molecular mechanisms causing variation in the timing of maturation are still poorly understood. Hence, investigation of whether a widespread mechanism like m6A methylation could be involved in controlling of the maturation timing is warranted. In salmon, two genes, also associated with age at maturity in humans, vgll3 and six6, have been shown to play an important role in maturation timing. In this study, we investigated the expression of 16 genes involved in the regulation of m6A RNA methylation in the hypothalamus of Atlantic salmon with different homozygous combinations of late and early alleles for vgll3 and six6 genes. We found differential expression of ythdf2.2, an m6A reader promoting mRNA degradation, with higher expression in six6*LL compared to other genotypes as well as in immature compared to mature males. In addition, we found that the expression levels of genes coding for an eraser, alkbh5, and for a reader, ythdf1, were higher in the hypothalamus of females than in males across all the different genotypes studied. However the total m6A levels between the whole hypothalamus of males and females were similar. Our results indicate a potential role of the m6A methylation process in sexual maturation of salmon, and provide the first evidence for such regulatory mechanism in the hypothalamus of any vertebrate
description: 34 pages, 5 figures
Delphinium peregrinum 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
Ranunculales
Ranunculaceae
Delphinium
Delphinium peregrinum

description: Delphinium peregrinum Linnaeus, Species Plantarum 1: 531. 1753.
"Habitat in Italia, Sicilia, Melita." RCN: 3949.
 Lectotype (Chowdhuri & Davis in Notes Roy. Bot. Gard. Edinburgh 22: 410. 1958): Herb. Clifford: 213, Delphinium 3 (BM-000628786).
 Generitype of Delphinium Linnaeus.
 Current name:  Delphinium peregrinum  L. (Ranunculaceae).
 Note: Delphinium peregrinum, with the type designated by Chowdhuri & Davis, was proposed as conserved type of the genus by Jarvis (in Taxon 41: 562. 1992). However, the proposal was eventually ruled unnecessary by the General Committee (see Barrie, l.c. 55: 795-796. 2006 for a review of the history of this and related proposals).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on pages 477-478, DOI: 10.5281/zenodo.291971
The Role of Ambipolar Diffusion in the Formation Process of Moderately Magnetized Diffuse Clouds
Creators: name: Inoue, Tsuyoshi
name: Inutsuka, Shu-ichiro
name: Koyama, Hiroshi
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the dynamical condensation process in a magnetized thermally bistable medium. We perform one-dimensional two fluid numerical simulations that describe the neutral and ionized components in the interstellar medium with purely transverse magnetic fields. We find that the clouds that are formed as a consequence of the thermal instability always have a magnetic field strength on the order of a few microgauss irrespective of the initial strength. This shows good agreement with the measurements of the magnetic field strength in diffuse clouds. We show analytically that the final magnetic field strength in the clouds is determined by the balance between ambipolar diffusion and the accumulation of the magnetic field due to condensation.
description: 4 pages, 4 figures, accepted for publication in the ApJL
The dynamical origin of multiple populations in intermediate-age clusters in the Magellanic Clouds
Creators: name: Hong, Jongsuk
name: de Grijs, Richard
name: Askar, Abbas
name: Berczik, Peter
name: Li, Chengyuan
name: Wang, Long
name: Deng, Licai
name: Kouwenhoven, M. B. N.
name: Giersz, Mirek
name: Spurzem, Rainer
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Numerical simulations were carried out to study the origin of multiple stellar populations in the intermediate-age clusters NGC 411 and NGC 1806 in the Magellanic Clouds. We performed NBODY6++ simulations based on two different formation scenarios, an ad hoc formation model where second-generation (SG) stars are formed inside a cluster of first-generation (FG) stars using the gas accumulated from the external intergalactic medium and a minor merger model of unequal mass ($M_{SG}$/$M_{FG}$ ~5-10%) clusters with an age difference of a few hundred million years. We compared our results such as the radial profile of the SG-to-FG number ratio with observations on the assumption that the SG stars in the observations are composed of cluster members, and confirmed that both the ad hoc formation and merger scenarios reproduce the observed radial trend of the SG-to-FG number ratio which shows less centrally concentrated SG than FG stars. It is difficult to constrain the formation scenario for the multiple populations by only using the spatial distribution of the SG stars. SG stars originating from the merger scenario show a significant velocity anisotropy and rotational features compared to those from the ad hoc formation scenario. Thus, observations aimed at kinematic properties like velocity anisotropy or rotational velocities for SG stars should be obtained to better understand the formation of the multiple populations in these clusters. This is, however, beyond current instrumentation capabilities.
description: 11 pages, 8 figures, 1 table; accepted for publication in MNRAS
Teleparallel theories of gravity as analogue of non-linear electrodynamics
Creators: name: Hohmann, Manuel
name: Järv, Laur
name: Krššák, Martin
name: Pfeifer, Christian
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The teleparallel formulation of gravity theories reveals close structural analogies to electrodynamics, which are more hidden in their usual formulation in terms of the curvature of spacetime. We show how every locally Lorentz invariant teleparallel theory of gravity with second order field equations can be understood as built from a gravitational field strength and excitation tensor which are related to each other by a constitutive relation, analogous to the axiomatic construction of theories of electrodynamics. We demonstrate how the previously studied models of $f(\mathbb{T})$ and $f(T_\text{ax},T_\text{ten},T_\text{vec})$ gravity as well as teleparallel dark energy can be formulated in this language. The advantage of this approach to gravity is that the field equations for different models all take the same compact form and general results can be obtained. An important new such result we find is a constraint which relates the field equations of the tetrad and the spin connection.
description: 13 pages, no figures; journal version
Additional file 1: of Epidemiology of heart failure in pediatric populations in low- and middle-income countries: a protocol for a systematic review
Creators: name: AurĂŠlie Sibetcheu
name: Valirie Agbor
name: Nyaga, Ulrich
name: Bigna, Jean
name: Noubiap, Jean
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: PRISMA-P. (DOCX 56Â kb)
Flight Sergeant Reg Bromhall North Africa
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: Reg Bromhall was a Flight Sergeant in the 92 squadron. On 7 January 1942, he was flying with a small formation of spitfires. When it encountered a large group of German aircraft. The squadron's diarist said it was the first prepared to stay and fight behind British lines since El Alamein. He was shot down along with Sergeant H Paterson. Neville Duke the famous World War 2 ace says the German planes were 109s. He also mentions they were from II/JG77. 2 German Pilots claimed they shot down spitfires that day Oberleutnant Lutz-Wilhelm Burckhardt (his 54th kill) and Leutnant Ernst Wilhelm Reinert. (his 105th kill) It was was of these 2 that shot down Reg Bromhall. Sgt Bromhall's life was saved by his parachute and in later life, he became a member of the Caterpillar Club for people whose lives have been saved by parachute. He was badly injured in the action and eventually had his leg amputated.Another member of the squadron at the time was Paul Brickhill who wrote The Dam Busters, Reach for the Sky and The Great Escape.
Anomalous Higgs Couplings at an $e γ$ Collider
Creators: name: Choudhury, Debajyoti
name: Mamta
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We examine the sensitivity of $e γ$ colliders (based on $e^+ e^-$ linear colliders of c.m. energy 500 GeV) to the anomalous couplings of the Higgs to W-bosons via the process $e^- γ\longrightarrow νW H$. This has the advantage over $e^+ e^-$ collider in being able to dissociate WWH vertex from ZZH. We are able to construct several dynamical variables which may be used to constrain vrious couplings in the WWH vertex.
description: 22 pages, 6 figures
Marginally compact fractal trees with semiflexibility
Creators: name: Dolgushev, Maxim
name: Hauber, Adrian L.
name: Pelagejcev, Philipp
name: Wittmer, Joachim P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We study marginally compact macromolecular trees that are created by means of two different fractal generators. In doing so, we assume Gaussian statistics for the vectors connecting nodes of the trees. Moreover, we introduce bond-bond correlations that make the trees locally semiflexible. The symmetry of the structures allows an iterative construction of full sets of eigenmodes (notwithstanding the additional interactions that are present due to semiflexibility constraints), enabling us to get physical insights about the trees' behavior and to consider larger structures. Due to the local stiffness the self-contact density gets drastically reduced.
description: 16 pages, 12 figures, accepted for publication in PRE
Eric Richard Hamlin
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: My father was on a tug by mistake at 14. A call came out to go to France to save our boys he told me about it the year before I lost him. It was both funny and sad.
Delphinium staphisagria 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
Ranunculales
Ranunculaceae
Delphinium
Delphinium staphisagria

description: Delphinium staphisagria Linnaeus, Species Plantarum 1: 531. 1753.
"Habitat in Istria, Dalmatia, Calabria, Apulia, Creta, Galloprovincia." RCN: 3952.
Type not designated.
Original material: none traced.
 Current name:  Delphinium staphisagria  L. (Ranunculaceae).
 Note: Munz (in J. Arnold Arbor. 48: 258. 1967) stated "Type locality: described from Istria, Dalmatia, Calabria, Apulia, S. France (LINN 694/12)", but did not explicitly treat the material as a type specimen. Ilarslan (in Turk. J. Bot. 20: 141. 1996) appears to follow him.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 478, DOI: 10.5281/zenodo.291971
G315.1+2.7: a new Galactic SNR from the AAO/UKST HAlpha survey
Creators: name: Stupar, M.
name: Parker, Q. A.
name: Filipovic, M. D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: New narrow-band HAlpha imaging and subsequent optical spectra confirm G315.1+2.7, a previously identified candidate supernova remnant (SNR), as a bona-fide Galactic SNR. Present observations are based on independent discovery of filamentary optical emission nebulosity on images of the AAO/UKST HAlpha survey of the southern Galactic plane which were found to co-incide with existing multi-frequency radio detections. Separate medium and high dispersion spectra were taken across two locations of this 11 arcmin N-S aligned optical filament. The resulting spectral signatures were found to strongly confirm the SNR identification based on standard emission line ratio discriminators which characterise emission from shock heated gas. The average observed ratios of [SII]/HAlpha=1.13, [NII]/HAlpha=1.43 and [SII] 6717/6731=1.46, together with the simultaneous detection of [OII] at 3727A, [OIII] 5007A and [OI] 6300A, all point to an SNR origin of the observed optical emission. Careful scrutiny of the low-resolution but high sensitivity SHASSA HAlpha survey also revealed a low-level but distinct optical emission arc. This arc precisely correlates with the large, 2.5 degree, north-south angular extent of the proposed new SNR also seen as a fractured structure in the extant radio data. G315.1+2.7 was detected previously at 2400 and 4800 MHz and at 408 and 1420 MHz. We also identified associated radio emission at 843 MHz from the now publicly available SUMSS survey. On the basis of optical imaging and spectra and radio observations at five frequencies, we identify G315.1+2.7 as a new Galactic SNR. The large projected angular extent of the new remnant, together with the distance estimate of ~1.7 kpc and diameter of ~80pc, make G315.1+2.7 one of the largest remnants known.
description: 10 pages, 10 figures. Accepted for MNRAS
Primordial non-Gaussianity in noncanonical warm inflation: three- and four-point correlations
Creators: name: Zhang, Xiao-Min
name: Ma, Hong-Yang
name: Chu, Peng-Cheng
name: Zhu, Jian-Yang
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Non-Gaussianity generated in inflation can be contributed by two parts. The first part, denoted by $f_{NL}^{δN}$, is the contribution from four-point correlation of inflaton field which can be calculated using $δN$ formalism, and the second part, denoted by $f_{NL}^{int}$, is the contribution from the three-point correlation function of the inflaton field. We consider the two contributions to the non-Gaussianity in noncanonical warm inflation throughout (noncanonical warm inflation is a new inflationary model which is proposed in \cite{Zhang2014}). We find the two contributions are complementary to each other. The four-point correlation contribution to the non-Gaussianity is overwhelmed by the three-point one in strong noncanonical limit, while the conclusion is opposite in the canonical case. We also discuss the influence of the field redefinition, thermal dissipative effect and noncanonical effect to the non-Gaussianity in noncanonical warm inflation.
description: 7 pages. Accepted for publication in Physical Review D
Two Loop QFT in the Making
Creators: name: Actis, Stefano
name: Passarino, Giampiero
name: Uccirati, Sandro
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recent developments in the evaluation of two-loop pseudo-observables and observables are briefly reviewed.
description: 5 pages, 2 figures, to appear in the proceedings of the 8th DESY Workshop on Elementary Particle Theory "Loops and Legs in Quantum Field Theory", April 2006, Eisenach, Germany
NUclei of GAlaxies: V. Radio emission in 7 NUGA sources
Creators: name: Krips, M.
name: Eckart, A.
name: Krichbaum, T. P.
name: Pott, J. -U.
name: Leon, S.
name: Neri, R.
name: Garcia-Burillo, S.
name: Combes, F.
name: Boone, F.
name: Baker, A. J.
name: Tacconi, L. J.
name: Schinnerer, E.
name: Hunt, L. K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high angular resolution radio snap-shot observations of seven nearby low-luminosity active galaxies (LLAGN) from the NUclei of GAlaxies (NUGA) survey. The observations were conducted with MERLIN and EVN/VLBI at 18cm and 6cm. At all observed angular resolutions and frequencies, we find indications for extended emission in about ~40% of the sources, consistent with the decrease of flux with increasing angular resolution. The extended components resemble jet emission in a majority of cases, consistent with the optically thin synchrotron emission implied by their steep spectra. We consider the compact 6cm EVN/VLBI radio emission of our sources in the context of the ``fundamental plane'' that previous LLAGN studies identified within the three-dimensional parameter space of radio luminosity, X-ray luminosity, and black hole mass. We demonstrate, using NGC7217 and NGC1068 as particular examples, that high-resolution, multi-epoch radio observations offer useful information about the origin of offsets from the fundamental plane.
description: Accepted for publication by A&A; 13 pages and 6 figures; Fig.5 & 6 have been revised
Constraints on the Progenitor of SN 2010jl and Pre-Existing Hot Dust in its Surrounding Medium
Creators: name: Dwek, Eli
name: Arendt, Richard G.
name: Fox, Ori D.
name: Kelly, Patrick L.
name: Smith, Nathan
name: Van Dyk, Schuyler D.
name: Filippenko, Alexei V.
name: Andrews, Jennifer
name: Shivvers, Isaac
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A search for the progenitor of SN~2010jl, an unusually luminous core-collapse supernova of Type~IIn, using pre-explosion {\it Hubble}/WFPC2 and {\it Spitzer}/IRAC images of the region, yielded upper limits on the UV and near-infrared (IR) fluxes from any candidate star. These upper limits constrain the luminosity and effective temperature of the progenitor, the mass of any preexisting dust in its surrounding circumstellar medium (CSM), and dust proximity to the star. A {\it lower} limit on the CSM dust mass is required to hide a luminous progenitor from detection by {\it Hubble}. {\it Upper} limits on the CSM dust mass and constraints on its proximity to the star are set by requiring that the absorbed and reradiated IR emission not exceed the IRAC upper limits. Using the combined extinction-IR emission constraints we present viable $M_d-R_1$ combinations, where $M_d$ and $R_1$ are the CSM dust mass and its inner radius. These depend on the CSM outer radius, dust composition and grain size, and the properties of the progenitor. The results constrain the pre-supernova evolution of the progenitor, and the nature and origin of the observed post-explosion IR emission from SN~2010jl. In particular, an $η$~Car-type progenitor will require at least 4~mag of visual extinction to avoid detection by the {\it Hubble}. This can be achieved with dust masses $\gtrsim 10^{-3}$~\msun\ (less than the estimated 0.2-0.5~\msun\ around $η$~Car) which must be located at distances of $\gtrsim 10^{16}$~cm from the star to avoid detection by {\it Spitzer}.
description: Accepted for publication in the ApJ. 14 pages 10 figures. The complete figure set for Figure 10 (24 images) is available in the online journal
Additional file 1: of Are dietary inequalities among Australian adults changing? a nationally representative analysis of dietary change according to socioeconomic position between 1995 and 2011â 13
Creators: name: Olstad, Dana
name: Leech, Rebecca
name: Livingstone, Katherine
name: Ball, Kylie
name: Thomas, Beth
name: Potter, Jane
name: Cleanthous, Xenia
name: Reynolds, Rachael
name: McNaughton, Sarah
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: 1995 National Nutrition Survey flow diagram. (PDF 10Â kb)
Cardamine bulbifera Crantz
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
Brassicales
Brassicaceae
Cardamine
Cardamine bulbifera

description: Dentaria bulbifera Linnaeus, Species Plantarum 2: 653. 1753.
"Habitat in Europa australi ad radices montium umbrosas." RCN: 4760.
 Lectotype (Marhold in Willdenowia 31: 45. 2001): Herb. Burser XVIII(1): 82 (UPS).
 Current name:  Cardamine bulbifera  (L.) Crantz (Brassicaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 478, DOI: 10.5281/zenodo.291971
Dear Dorothy
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: Attached is a book that I have produced of my grandad's letters sent to my Nan during WWII. These range from 1940 when he first went into training in Winchester until he returned home in 1946 after finally being released from the Army. The letters follow him through his initial training, being posted to Egypt and being captured as a Prisoner of War. He was kept at the camp which was the first camp to be liberated.
Comments on the Relativity of Shape
Creators: name: Hoyer, Paul
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this talk I address three topics related to the shape of hadrons: 1. The Lorentz contraction of bound states. Few dedicated studies of this exist - I describe a recent calculation for ordinary atoms (positronium). 2. Does the A-dependence of nuclear structure functions indicate a change of proton shape in the nuclear environment? (My short answer is no.) 3. The size of Fock states contributing to processes involving large momentum transfers. End-point configurations can be transversally extended and yet sufficiently short-lived to contribute coherently to hard scattering.
description: Talk at the Workshop on the Shape of Hadrons, 27-29 April 2006 in Athens, Greece. 11 pages, 15 figures
Buteo platypterus
Creators: name: Pedroza, Diego
name: Melo, Tomaz Nascimento de
name: Machado, Tatiana Lemos da Silva
name: Guimarães, David Pedroza
name: Lima, Jônatas M.
name: Guilherme, Edson
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Accipitriformes
Accipitridae
Buteo
Buteo platypterus

description: BROAD-WINGED HAWK Buteo platypterus
 Nearctic migrant. Observed by DP at the edge of HFR on 9 November 2017 (WA2792378; Fig. 2A). Only the second record in Acre (Guilherme 2016). Stot et al. (1992) reported the species’ occurrence in neighbouring Rondônia between October and March. This indicates that the record at HFR was within its overwintering period in south-west Amazonia.
description: Published as part of Pedroza, Diego, Melo, Tomaz Nascimento de, Machado, Tatiana Lemos da Silva, Guimarães, David Pedroza, Lima, Jônatas M. & Guilherme, Edson, 2020, Birds of Humaitá Forest Reserve, Acre, Brazil: an important forest fragment in south-west Amazonia, pp. 58-79 in Bulletin of the British Ornithologists' Club 140 (1) on page 61, DOI: 10.25226/bboc.v140i1.2020.a7, http://zenodo.org/record/12535635
Cardamine enneaphyllos R. Br.
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
Brassicales
Brassicaceae
Cardamine
Cardamine enneaphyllos

description: Dentaria enneaphyllos Linnaeus, Species Plantarum 2: 653. 1753.
"Habitat in Austria, Italia." RCN: 4759.
 Lectotype (Marhold in Willdenowia 31: 44. 2001): Herb. Burser XVIII(1): 83 (UPS).
 Current name:  Cardamine enneaphyllos  (L.) R. Br. (Brassicaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 478, DOI: 10.5281/zenodo.291971
Voluntary Civil Support and Dorking in Wartime for a 7-year-old
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: Story 1 (see file) is a record of the Mayor of Chipping Norton proactively organising the town in preparation for war, and subsequently welcoming evacuees, then survivors from Dunkirk. Moving to Dorking in the middle of the Battle of Britain for unknown activities.Story 2 (see file) relates to my experiences as a 7-12 year old in Dorking during the war.
Optimized Pre-Compensating Compression
Creators: name: Dar, Yehuda
name: Elad, Michael
name: Bruckstein, Alfred M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Multimedia (cs.MM)
subject: FOS: Computer and information sciences

description: In imaging systems, following acquisition, an image/video is transmitted or stored and eventually presented to human observers using different and often imperfect display devices. While the resulting quality of the output image may severely be affected by the display, this degradation is usually ignored in the preceding compression. In this paper we model the sub-optimality of the display device as a known degradation operator applied on the decompressed image/video. We assume the use of a standard compression path, and augment it with a suitable pre-processing procedure, providing a compressed signal intended to compensate the degradation without any post-filtering. Our approach originates from an intricate rate-distortion problem, optimizing the modifications to the input image/video for reaching best end-to-end performance. We address this seemingly computationally intractable problem using the alternating direction method of multipliers (ADMM) approach, leading to a procedure in which a standard compression technique is iteratively applied. We demonstrate the proposed method for adjusting HEVC image/video compression to compensate post-decompression visual effects due to a common type of displays. Particularly, we use our method to reduce motion-blur perceived while viewing video on LCD devices. The experiments establish our method as a leading approach for preprocessing high bit-rate compression to counterbalance a post-decompression degradation.
Longevity of supersymmetric flat directions
Creators: name: Allahverdi, Rouzbeh
name: Mazumdar, Anupam
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We examine the fate of supersymmetric flat directions. We argue that the non-perturbative decay of the flat direction via preheating is an unlikely event. In order to address this issue, first we identify the physical degrees of freedom and their masses in presence of a large flat direction VEV (Vacuum Expectation Value). We explicitly show that the (complex) flat direction and its fermionic partner are the only light {\it physical} fields in the spectrum. If the flat direction VEV is much larger than the weak scale, and it has a rotational motion, there will be no resonant particle production at all. The case of multiple flat directions is more involved. We illustrate that in many cases of physical interest, the situation becomes effectively the same as that of a single flat direction, or collection of independent single directions. In such cases preheating is not relevant. In an absence of a fast non-perturbative decay, the flat direction survives long enough to affect thermalization in supersymmetric models as described in hep-ph/0505050 and hep-ph/0512227. It can also ``terminate'' an early stage of non-perturbative inflaton decay as discussed in hep-ph/0603244.
description: 9 revtex pages, v3: expanded discussion on two flat directions, minor modifications, conclusions unchanged
Detectability of dark matter subhalos by means of the GAMMA-400 telescope
Creators: name: Egorov, A. E.
name: Galper, A. M.
name: Topchiev, N. P.
name: Leonov, A. A.
name: Suchkov, S. I.
name: Kheymits, M. D.
name: Yurkin, Yu. T.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigated the detectability of Galactic subhalos with masses $(10^6-10^9)M_{\odot}$ formed by annihilating WIMP dark matter by the planned GAMMA-400 gamma-ray telescope. The inner structure of dark matter subhalos and their distribution in the Galaxy were taken from corresponding simulations. We showed that the expected gamma-ray flux from subhalos strongly depends on WIMP mass and subhalo concentration, but less strongly depends on the subhalo mass. In an optimistic case we may expect the flux of 10-100 ph/year above 100 MeV from the closest and most massive subhalos, which would be detectable sources for GAMMA-400. However, resolving the inner structure of subhalos might be possible only by the joint analysis of the future GAMMA-400 data and data from other telescopes due to smallness of fluxes. Also we considered the recent subhalo candidates 3FGL J2212.5+0703 and J1924.8-1034 within the framework of our model. We concluded that it is very unlikely that these sources belong to the subhalo population.
description: Was presented at International Symposium on Cosmic Rays and Astrophysics (ISCRA-2017), 20-22 June 2017, Moscow, Russia
Poem in Memory of My Father
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: Every now and then I think - we never said hello. No sooner had we met then you must go, to travel miles across a world where sombre banners were unfurled and armies clashed across the mountains and the streams. Where dying screams were all around. I would have liked to walk with you, to smile and take your hands, to understand. But I was just a babe when you came home, to stay awhile then leave alone, never to return. When will they learn? Wars bring no resolution. No solution. And those who have to go? They know. Sleep well. Thankyou for facing the hell, for all of us. God bless
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Cart. 193 (11 H 78), f. 0225v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0225v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0225v, 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