cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Cart. 187 (11 H 72), f. 0066v
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: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0066v, 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 III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0066v, 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
Assessing the massive young Sun hypothesis to solve the warm young Earth puzzle
Creators: name: Minton, David A.
name: Malhotra, Renu
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A moderately massive early Sun has been proposed to resolve the so-called faint early Sun paradox. We calculate the time-evolution of the solar mass that would be required by this hypothesis, using a simple parametrized energy-balance model for Earth's climate. Our calculations show that the solar mass loss rate would need to have been 2-3 orders of magnitude higher than present for a time on the order of ~2 Gy. Such a mass loss history is significantly at variance (both in timescale and in the magnitude of the mass loss rates) with that inferred from astronomical observations of mass loss in younger solar analogues. While suggestive, the astronomical data cannot completely rule out the possibility that the Sun had the required mass loss history; therefore, we also examine the effects of the hypothetical historical solar mass loss on orbital dynamics in the solar system, with a view to identifying additional tests of the hypothesis. Planetary and satellite orbits provide a few tests, but these are weak or non-unique.
description: 19 pages, 4 figures, 1 table; submitted to ApJ on Dec. 8, 2006
Life of Π
Creators: name: Maier, Andreas
name: Marquard, Peter
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The heavy-quark contribution to the polarisation function $Π$ at higher perturbative orders is presently only known approximately. We scrutinise the accuracy of state-of-the-art approximations at three- and four-loop order. At three loops, we present for the first time a result with arbitrary numerical precision for general kinematics and compare to the best Padé estimate. At four loops, we calculate the fourth (inverse) moment of the non-singlet heavy-quark vacuum polarisation in order to test the prediction for this moment based on Padé approximation.
description: 21 pages, 2 figures. Equivalent to journal version
Reconciling large CP-violating phases with bounds on the electric dipole moments in the MSSM
Creators: name: Ayazi, Seyed Yaser
name: Farzan, Yasaman
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The possibility of cancelation between different contributions to d_e, d_n and d_{Hg} has been reconsidered with special emphasis on the region that is phenomenologically interesting (intermediate values of \tan βand sub-TeV sfermion masses). It is found that in the range favored by electroweak baryogenesis (\it i.e., |μ|\simeq M_1 or |μ|\simeq M_2), \sin [θ_μ+θ_{M_1}]\sim 1 can be compatible with the EDM bounds even for slepton masses below 500 GeV. Such large values of the phases promise a successful electroweak baryogenesis. The possibility of large CP-odd effects at linear collider has also been discussed.
description: 33 pages, 12 figures
Addendum to ``Threshold corrections to $m_b$ and the $\bar{b}b \to H^0_i$ production in CP-violating SUSY scenarios''
Creators: name: Borzumati, Francesca
name: Lee, Jae Sik
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In hep-ph/0401024: ``Threshold corrections to $m_b$ and the $\bar{b}b\to H^0_i$ production in CP-violating SUSY scenarios'', we have pointed out that the production cross sections of the three neutral Higgs bosons through $\bar{b}b$ fusion can deviate substantially from those obtained in CP conserving scenarios, thanks to the nontrivial role played by the threshold corrections to $m_b$ combined with the CP-violating mixing in the neutral-Higgs-boson sector. The deviations are largest for values of the CP-violating phases that maximize the mixing among at least two of the three neutral Higgs bosons. We complement our previous work focussing explicitly on the values of masses and widths of the three neutral Higgs bosons in this region of parameter space. We then address the issue of whether the three different peaks in the invariant mass distribution of the Higgs-decay products can be experimentally disentangled at the LHC.
description: 1+6 pages, 3 figures
Non-Count Symmetries in Boolean & Multi-Valued Prob. Graphical Models
Creators: name: Anand, Ankit
name: Noothigattu, Ritesh
name: Singla, Parag
name: Mausam
Publisher: name: arXiv
Year: 2017
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Lifted inference algorithms commonly exploit symmetries in a probabilistic graphical model (PGM) for efficient inference. However, existing algorithms for Boolean-valued domains can identify only those pairs of states as symmetric, in which the number of ones and zeros match exactly (count symmetries). Moreover, algorithms for lifted inference in multi-valued domains also compute a multi-valued extension of count symmetries only. These algorithms miss many symmetries in a domain. In this paper, we present first algorithms to compute non-count symmetries in both Boolean-valued and multi-valued domains. Our methods can also find symmetries between multi-valued variables that have different domain cardinalities. The key insight in the algorithms is that they change the unit of symmetry computation from a variable to a variable-value (VV) pair. Our experiments find that exploiting these symmetries in MCMC can obtain substantial computational gains over existing algorithms.
description: 9 pages, 5 figures
Equation of state for distributed mass quark matter
Creators: name: Biro, T. S.
name: Levai, P.
name: Van, P.
name: Zimanyi, J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate how the QCD equation of state can be reconstructed by a continous mass distribution of non-interacting ideal components. We find that adjusting the mass scale as a function of the temperature leads to results which are conform to the quasiparticle model, but a temperature independent distribution also may fit lattice results. The fitted mass distribution tends to show a mass gap, supporting the physical picture of the quark coalescence in hadronization.
description: talk given at SQM2006, 8 pages, submitted to J.Phys.G
MOESM2 of CHRNA5 and CHRNA3 polymorphism and lung cancer susceptibility in Palestinian population
Creators: name: Ayesh, Basim
name: Al-Masri, Rami
name: Abed, Abdalla
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: Additional file 2. Genotype distribution of the SNP rs16969968 and the SNP rs1051730 among cases and controls.
Hirschfeldia incana Lagr.
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
Hirschfeldia
Hirschfeldia incana

description: Sinapis incana Linnaeus, Centuria I Plantarum: 19. 1755.
"Habitat in Gallia, Lusitania, Hispania." RCN: 4871.
 Lectotype (Gómez-Campo in Cafferty & Jarvis in Taxon 51: 535. 2002): [icon] "Erysimum brevissimis siliquis subincanum" in Hermann, Parad. Bat.: 155. 1698.
 Current name:  Hirschfeldia incana  (L.) Lagr. -Foss. (Brassicaceae).
 Note: Jafri (in Fl. Libya 23 : 27. 1977) designated Herb. Linn. No. 845.16 (LINN) as type, evidently unaware that the material is identifiable as Brassica nigra (L.) Koch. The other original element, however, the cited Hermann plate, does correspond with current usage. Although there are few characters in the protologue that allow the two taxa to be distinguished, Linnaeus (1755: 20) did refer to "Folia canescentia", a character pointing strongly to H. incana but not to B. nigra. Gómez-Campo therefore rejected Jafri’s typification in favour of the Hermann plate, in accordance with Art. 9.17 (b), in order to preserve nomenclatural stability.
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 853, DOI: 10.5281/zenodo.291971
Oscillation effects on high-energy neutrino fluxes from astrophysical hidden sources
Creators: name: Mena, Olga
name: Mocioiu, Irina
name: Razzaque, Soebur
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: High-energy neutrinos are expected to be produced in a vareity of astrophysical sources as well as in optically thick hidden sources. We explore the matter-induced oscillation effects on emitted neutrino fluxes of three different flavors from the latter class. We use the ratio of electron and tau induced showers to muon tracks, in upcoming neutrino telescopes, as the principal observable in our analysis. This ratio depends on the neutrino energy, density profile of the sources and on the oscillation parameters. The largely unknown flux normalization drops out of our calculation and only affects the statistics. For the current knowledge of the oscillation parameters we find that the matter-induced effects are non-negligible and the enhancement of the ratio from its vacuum value takes place in an energy range where the neutrino telescopes are the most sensitive. Quantifying the effect would be useful to learn about the astrophysics of the sources as well as the oscillation parameters. If the neutrino telescopes mostly detect diffuse neutrinos without identifying their sources, then any deviation of the measured flux ratios from the vacuum expectation values would be most naturally explained by a large population of hidden sources for which matter-induced neutrino oscillation effects are important.
description: Phys.Rev.D accepted version. 12 pages, 10 figures. Results unchanged, added references, minor changes and text re-arrangements
Low Metallicities and Old Ages for Three Ultra-Diffuse Galaxies in the Coma Cluster
Creators: name: Gu, Meng
name: Conroy, Charlie
name: Law, David
name: van Dokkum, Pieter
name: Yan, Renbin
name: Wake, David
name: Bundy, Kevin
name: Merritt, Allison
name: Abraham, Roberto
name: Zhang, Jielai
name: Bershady, Matthew
name: Bizyaev, Dmitry
name: Brinkmann, Jonathan
name: Drory, Niv
name: Grabowski, Kathleen
name: Masters, Karen
name: Pan, Kaike
name: Parejko, John
name: Weijmans, Anne-Marie
name: Zhang, Kai
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A large population of ultra-diffuse galaxies (UDGs) was recently discovered in the Coma cluster. Here we present optical spectra of three such UDGs, DF7, DF44 and DF17, which have central surface brightnesses of $μ_g \approx 24.4-25.1$ mag arcsec$^{-2}$. The spectra were acquired as part of an ancillary program within the SDSS-IV MaNGA Survey. We stacked 19 fibers in the central regions from larger integral field units (IFUs) per source. With over 13.5 hours of on-source integration we achieved a mean signal-to-noise ratio (S/N) in the optical of $9.5$Å$^{-1}$, $7.9$Å$^{-1}$ and $5.0$Å$^{-1}$, respectively, for DF7, DF44 and DF17. Stellar population models applied to these spectra enable measurements of recession velocities, ages and metallicities. The recession velocities of DF7, DF44 and DF17 are $6599^{+40}_{-25}$km/s, $6402^{+41}_{-39}$km/s and $8315^{+43}_{-43}$km/s, spectroscopically confirming that all of them reside in the Coma cluster. The stellar populations of these three galaxies are old and metal-poor, with ages of $7.9^{+3.6}_{-2.5}$Gyr, $8.9^{+4.3}_{-3.3}$Gyr and $9.1^{+3.9}_{-5.5}$Gyr, and iron abundances of $\mathrm{[Fe/H]}$ $-1.0^{+0.3}_{-0.4}$, $-1.3^{+0.4}_{-0.4}$ and $-0.8^{+0.5}_{-0.5}$, respectively. Their stellar masses are $3$-$6\times10^8 M_\odot$. The UDGs in our sample are as old or older than galaxies at similar stellar mass or velocity dispersion (only DF44 has an independently measured dispersion). They all follow the well-established stellar mass$-$stellar metallicity relation, while DF44 lies below the velocity dispersion-metallicity relation. These results, combined with the fact that UDGs are unusually large for their stellar mass, suggest that stellar mass plays a more important role in setting stellar population properties for these galaxies than either size or surface brightness.
description: 13 pages, 12 figures, published in ApJ
Additional file 1: of Video as a mediating artefact of science learning: cogenerated views of what helps students learn from watching video
Creators: name: Higgins, Joanna
name: Moeed, Azra
name: Raewyn Eden
Publisher: name: figshare
Year: 2018
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Maori abstract. (DOCX 17Â kb)
2dF-SDSS LRG and QSO (2SLAQ) Survey: Evolution of the Most Massive Galaxies
Creators: name: Nichol, Robert
name: Cannon, Russell
name: Roseboom, Isaac
name: Wake, David
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The 2dF-SDSS LRG and QSO (2SLAQ) survey is a new survey of distant Luminous Red Galaxies (LRGs) and faint quasars selected from the Sloan Digital Sky Survey (SDSS) multi-color photometric data and spectroscopically observed using the 2dF instrument on the Anglo-Australian Telescope (AAT). In total, the 2SLAQ survey has measured over 11000 LRG redshifts, covering 180deg^2 of SDSS imaging data, from 87 allocated nights of AAT time. Over 90% of these galaxies are within the range 0.45=3L*. When combined with the lower redshift SDSS LRGs, the evolution in the luminosity function of these LRGs is fully consistent with that expected from a simple passive (luminosity) evolution model. This observation suggests that at least half of the LRGs seen at z~0.2 must already have more than half their stellar mass in place by z~0.6, i.e., our observations are inconsistent with a majority of LRGs experiencing a major merger in the last 6 Gyrs. However, some "frosting" (i.e., minor mergers) has taken place with ~5% of LRGs showing some evidence of recent and/or on-going star-formation, but it only contributes ~1% of their stellar mass.
description: Proceedings for the conference "Heating vs. Cooling in Galaxies and Clusters of Galaxies", August 2006, Garching, Germany. See the 2SLAQ website at http://www.2slaq.info
Detection strategies for the first supernovae with JWST
Creators: name: Hartwig, Tilman
name: Bromm, Volker
name: Loeb, Abraham
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Pair-instability supernovae (PISNe) are very luminous explosions of massive, low metallicity stars. They can potentially be observed out to high redshifts due to their high explosion energies, thus providing a probe of the Universe prior to reionization. The near-infrared camera, NIRCam, on board the James Webb Space Telescope is ideally suited for detecting their redshifted ultraviolet emission. We calculate the photometric signature of high-redshift PISNe and derive the optimal detection strategy for identifying their prompt emission and possible afterglow. We differentiate between PISNe and other sources that could have a similar photometric signature, such as active galactic nuclei or high-redshift galaxies. We demonstrate that the optimal strategy, which maximizes the visibility time of the PISN lightcurve per invested exposure time, consists of the two wide-band filters F200W and F356W with an exposure time of 600s. For such exposures, we expect one PISN at $z \lesssim 7.5$ per at least 50,000 different field of view, which can be accomplished with parallel observations and an extensive archival search. The PISN afterglow, caused by nebular emission and reverberation, is very faint and requires unfeasibly long exposure times to be uniquely identified. However, this afterglow would be visible for several hundred years, about two orders of magnitude longer than the prompt emission, rendering PISNe promising targets for future, even more powerful telescopes.
description: 13 pages, 9 figures, 2 tables, submitted to MNRAS
Lettre de Jean-Pierre Papon à Jean-François Séguier, 1777-10-31
Creators: name: Papon, Jean-Pierre
name: Papon, Jean-Pierre
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021

description: [transcription] Monsieur,

Je voudrais savoir si le marc de Montpellier, en 1309, avant même cette époque et après, n’était pas au marc de France comme 56 2/3 à 58. C’est du moins ce qui est résulté en quelques recherches que j’ai faites sur cette matière. Je m’adresse à vous avec confiance, parce que je compte sur vos lumières et sur votre complaisance. Peut-être votre marc actuel conserve-t-il la même proportion qu’autrefois relativement au marc de Provence. Quand on veut le débrouiller, l’approfondir et la mettre dans un jour à pouvoir le faire lire, et surtout quand on est tout seul pour un travail de cette espèce, la rédaction seule, les matériaux et la difficulté de séparer tous les objets pour les mettre chacun à leur place, occuperaient un homme. À vos moments de loisirs, quand vous aurez quelques observations à me faire sur le 1er volume, je vous prie de me les envoyer et de compter toujours sur le sincère attachement que je vous ai voué pour la vie et avec lequel j’ai l’honneur d’être, Monsieur, votre très humble et très obéissant serviteur.

Papon, de l’Oratoire.

Marseille, le 31 octobre 1777.
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 147_6, fol. 97
description: Source: ark:/12148/btv1b10015294z
Brassica juncea Czern.
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
Brassica
Brassica juncea

description: Sinapis juncea Linnaeus, Species Plantarum 2: 668. 1753.
"Habitat in Asia." RCN: 4868.
 Lectotype (Bailey in Gentes Herb. 1: 95. 1922): Herb. Linn. No. 845.11 (LINN).
 Current name:  Brassica juncea  (L.) Czern. (Brassicaceae).
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 854, DOI: 10.5281/zenodo.291971
Self-consistent variational approach to the minimal left-right symmetric model of electroweak interactions
Creators: name: Siringo, Fabio
name: Marotta, Luca
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The problem of mass generation is addressed by a Gaussian variational method for the minimal left-right symmetric model of electroweak interactions. Without any scalar bidoublet, the Gaussian effective potential is shown to have a minimum for a broken symmetry vacuum with a finite expectation value for both the scalar Higgs doublets. The symmetry is broken by the fermionic coupling that destabilizes the symmetric vacuum, yielding a self consistent fermionic mass. In this framework a light Higgs is only compatible with the existence of a new high energy mass scale below 2 TeV.
description: 5 pages, 3 figures. New comments added and typing errors in eq. 8 and 11 corrected
Design of Decoupling and Nonlinear PD Controller for Cruise Control of a Quadrotor
Creators: name: Arrosida, Hanum
name: Effendi, Rusdhianto
name: Agustinah, Trihastuti
name: Pramudijanto, Josaphat
Publisher: name: arXiv
Year: 2017
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Quadrotor is often used to accomplish various missions related to surveillance, territory mapping, search and rescue, and other purposes. Quadrotor is a nonlinear system with multiple input multiple output and has stability issue due to external disturbance. These characteristics lead to difficulty in cruise control of quadrotor automatically. Decoupling method is used to eliminate the interaction of other control on rotational motion, then the roll, pitch, and yaw angle can be controlled independently. Nonlinear PD controller is obtained from invers model of control signal on a quad rotor and it is used to control the translational motion in x and y axis with nonlinear dynamics because of the influence the rotational angle. Simulation results show that the proposed method can eliminate the control interaction of roll, pitch and yaw angle, hence it works like single input single output system and translational motion on x andy axis can achieve the expected trajectory precisely.
description: Published in: 2015 International Seminar on Intelligent Technology and Its Applications
MOESM1 of Abundance of adverse environmental conditions during critical stages of crop production in Northern Germany
Creators: name: Strer, Maximilian
name: Svoboda, Nikolai
name: Herrmann, Antje
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: Developmental Biology

description: Additional file 1. Suppl Materials 1â 4.
The Shape of the Gravitational Potential in Cold Dark Matter Halos
Creators: name: Hayashi, E.
name: Navarro, J. F.
name: Springel, V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a set of cosmological N-body simulations to investigate the structural shape of galaxy-sized cold dark matter (CDM) halos. Unlike most previous work on the subject - which dealt with shapes as measured by the inertia tensor - we focus here on the shape of the gravitational potential, a quantity more directly relevant to comparison with observational probes. A further advantage is that the potential is less sensitive to the effects of substructure and, as a consequence, the isopotential surfaces are typically smooth and well approximated by concentric ellipsoids. Our main result is that the asphericity of the potential increases rapidly towards the center of the halo. The radial trend is more pronounced than expected from constant flattening in the mass distribution, and reflects a strong tendency for dark matter halos to become increasingly aspherical inwards. Near the center the halo potential is approximately prolate ((c/a)_0=0.72 +/- 0.04, (b/a)_0=0.78 +/- 0.08), but it becomes increasingly spherical in the outer regions. The principal axes of the isopotential surfaces remain well aligned, and in most halos the angular momentum tends to be parallel to the minor axis and perpendicular to the major axis. This suggests that galactic disks may form in a plane where the potential is elliptical and where its ellipticity varies rapidly with radius. This can result in significant deviations from circular motion in systems such as low surface brightness galaxies (LSBs), even for relatively minor deviations from circular symmetry. Simulated long-slit rotation curves can appear similar to those of LSBs often cited as evidence for constant density "cores". This suggests that taking into account the 3D shape of the dark mass distribution might help to reconcile such evidence with the cuspy mass profile of CDM halos.
description: 18 pages, 10 figures, accepted by MNRAS after minor revisions, high resolution version avaliable at http://www.mpa-garching.mpg.de/~ehayashi/potshape
Clockwork Higgs portal model for freeze-in dark matter
Creators: name: Kim, Jinsu
name: McDonald, John
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The clockwork mechanism can explain interactions which are dimensionally very weak without the need for very large mass scales. We present a model in which the clockwork mechanism generates the very small Higgs portal coupling and dark matter particle mass necessary to explain cold dark matter via the freeze-in mechanism. We introduce a TeV-scale scalar clockwork sector which couples to the Standard Model via the Higgs portal. The dark matter particle is the lightest scalar of the clockwork sector. We show that the freeze-in mechanism is dominated by decay of the heavy clockwork scalars to light dark matter scalars and Higgs bosons. In the model considered, we find that freeze-in dark matter is consistent with the clockwork mechanism for global charge $q$ in the range $2 \lesssim q \lesssim 4$ when the number of massive scalars is in the range $10 \leq N \leq 20$. The dark matter scalar mass and portal coupling are independent of $q$ and $N$. For a typical TeV-scale clockwork sector, the dark matter scalar mass is predicted to be of the order of a MeV.
description: v3: To be published in PRD
Bounding the magnetic and electric dipole moments of tau nu from the process e+e- --> nu bar nu gamma in E6 Superstring Models
Creators: name: Gutierrez-Rodriguez, A.
name: Hernandez-Ruiz, M. A.
name: Jayme-Valdes, B.
name: Perez, M. A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We obtain bounds on the anomalous magnetic and electric dipole moments of the tau-neutrino through the reaction $e^{+}e^{-}\to ν\bar νγ$ at the $Z_1$-pole in the framework of a Left-Right symmetric model and a class of $E_6$ inspired models with an additional neutral vector boson $Z_θ$. We use the data collected by the L3 Collaboration at LEP. For the parameters of the $E_6$ model we consider the mixing angle $θ_{E_6}=37.8^o$ and $M_{Z_θ}=7M_{Z_1}$. We find that our bounds are of the same order of magnitude as those obtained in other extensions of the Standard Model.
description: 17 pages, 2 figure
SHOC2 phosphatase-dependent RAF dimerization mediates resistance to MEK inhibition in RAS-mutant cancers.
Creators: name: Jones, Greg G
name: Río, Isabel Boned Del
name: Sari, Sibel
name: Aysen Sekerim
name: Young, Lucy C
name: Hartig, Nicole
name: Zubiaur, Itziar Areso
name: El-Bahrawy, Mona A
name: Hynds, Rob E
name: Lei, Winnie
name: Arcas, Miriam Molina
name: Downward, Julian
name: Rodriguez-Viciana, Pablo
Publisher: name: The Francis Crick Institute
Year: 2020
Subjects: Model organisms
Tumour Biology
Signalling & Oncogenes
Gene Expression
Genetics & Genomics
Chemical Biology & High Throughput

description: Targeted inhibition of the ERK-MAPK pathway, upregulated in a majority of human cancers, has been hindered in the clinic by drug resistance and toxicity. The MRAS-SHOC2-PP1 (SHOC2 phosphatase) complex plays a key role in RAF-ERK pathway activation by dephosphorylating a critical inhibitory site on RAF kinases. Here we show that genetic inhibition of SHOC2 suppresses tumorigenic growth in a subset of KRAS-mutant NSCLC cell lines and prominently inhibits tumour development in autochthonous murine KRAS-driven lung cancer models. On the other hand, systemic SHOC2 ablation in adult mice is relatively well tolerated. Furthermore, we show that SHOC2 deletion selectively sensitizes KRAS- and EGFR-mutant NSCLC cells to MEK inhibitors. Mechanistically, SHOC2 deletion prevents MEKi-induced RAF dimerization, leading to more potent and durable ERK pathway suppression that promotes BIM-dependent apoptosis. These results present a rationale for the generation of SHOC2 phosphatase targeted therapies, both as a monotherapy and to widen the therapeutic index of MEK inhibitors.
Erucastrum virgatum C. Presl
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
Erucastrum
Erucastrum virgatum

description: Sinapis laevigata Linnaeus, Centuria I Plantarum: 20. 1755.
"Habitat in Lusitania, Hispania." RCN: 4872.
Type not designated.
Original material: Herb. Linn. No. 845.17 (LINN); [icon] in Hermann, Parad. Bat.: 155. 1698.
 Current name:  Erucastrum virgatum  C. Presl (Brassicaceae).
 Note: This name has been informally rejected as a nomen ambiguum by the majority of recent authors.
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 854, DOI: 10.5281/zenodo.291971
Brassica nigra W. D. J. Koch
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
Brassica
Brassica nigra

description: Sinapis nigra Linnaeus, Species Plantarum 2: 668. 1753.
"Habitat in aggeribus ruderatis Europae septentrionalioris." RCN: 4864.
 Lectotype (Jonsell & Jarvis in Nordic J. Bot. 22: 71. 2002): Herb. Clifford: 338, Sinapis 2 (BM-000646359).
 Current name:  Brassica nigra  (L.) W.D.J. Koch (Brassicaceae).
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 854, DOI: 10.5281/zenodo.291971
Additional file 4: of A gel-based PCR method to differentiate sheeppox virus field isolates from vaccine strains
Creators: name: Tesfaye Chibssa
name: Grabherr, Reingard
name: Loitsch, Angelika
name: Tirumala Settypalli
name: Tuppurainen, Eeva
name: Nwankpa, Nick
name: Tounkara, Karim
name: Madani, Hafsa
name: Omani, Amel
name: Diop, Mariane
name: Cattoli, Giovanni
name: Diallo, Adama
name: Lamien, Charles
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S3. Gel picture of PCR for the non-capripoxvirus samples tested in this study. MM = 50 bp DNA ladder; a = positive control plasmid of the SPPV field isolates; b = positive control plasmid of the SPPV vaccine strain; c = Negative control; 1–5 (ORF viruses); 6 (BPSV); 7–8 (Mccp); 9 (cDNA, PPRV); 10 (BOHV-1); 11 (BOHV-2). (PDF 45 kb)
Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation
Creators: name: Pan, Kuo-Chuan
name: Liebendörfer, Matthias
name: Couch, Sean M.
name: Thielemann, Friedrich-Karl
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate axisymmetric black hole~(BH) formation and its gravitational wave (GW) and neutrino signals with self-consistent core-collapse supernova simulations of a non-rotating $40~M_\odot$ progenitor star using the isotropic diffusion source approximation for the neutrino transport and a modified gravitational potential for general relativistic effects. We consider four different neutron star (NS) equations of state~(EoS): LS220, SFHo, BHB$Λϕ$ and DD2, and study the impact of the EoS on BH formation dynamics and GW emission. We find that the BH formation time is sensitive to the EoS from 460 to $>1300$~ms and is delayed in multiple dimensions for $\sim~100-250$~ms due to the finite entropy effects. Depending on the EoS, our simulations show the possibility that shock revival can occur along with the collapse of the proto-neutron star~(PNS) to a BH. The gravitational waveforms contain four major features that are similar to previous studies but show extreme values: (1)~a low frequency signal ($\sim~300-500$~Hz) from core-bounce and prompt convection, (2)~a strong signal from the PNS g-mode oscillation among other features, (3)~a high frequency signal from the PNS inner-core convection, and (4)~signals from the standing accretion shock instability and convection. The peak frequency at the onset of BH formation reaches to $\sim~2.3$~kHz. The characteristic amplitude of a 10~kpc object at peak frequency is detectable but close to the noise threshold of the Advanced~LIGO and KAGRA, suggesting that the next generation gravitational wave detector will need to improve the sensitivity at the kHz domain to better observe stellar-mass BH formation from core-collapse supernovae or failed supernovae.
description: 8 figures. Accepted by ApJ
Sinapis arvensis var. orientalis 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
Brassicales
Brassicaceae
Sinapis
Sinapis arvensis
Sinapis arvensis l. var. orientalis (l.) w.d.j. koch & ziz

description: Sinapis orientalis Linnaeus, Centuria I Plantarum: 19. 1755.
"Habitat in Oriente." RCN: 4861.
 Lectotype (Hedge in Cafferty & Jarvis in Taxon 51: 535. 2002): Herb. Linn. No. 845.3 (LINN).
 Current name:  Sinapis arvensis  L. var.  orientalis  (L.) W.D.J. Koch & Ziz (Brassicaceae).
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 854, DOI: 10.5281/zenodo.291971
Story of Frank George Foote (Royal Army Service Corps)
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: Frank was born in London in 1904 and lived in Camberwell. The interviewee's father's mother left his father (who was roughly 8 years old at the time of the war) in a children's home but his aunt got him out of the home and looked after him. Frank joined up in October 1942 because there was a shortage of officers. He did various courses, including a motorcycle course. He became a Captain in the Royal Army Service Corps. After the war, he returned to civilian life as an insurance broker and went around assessing war damage. Frank never talked much about the war, but he did talk about an incident with the Belgians.To escape the Blitz, the family moved to a farm-house in Long Crendon, where there was a searchlight on a nearby hill. Late one night, they heard the drone of an aircraft engine. His father was in the corps for recognising aircraft silhouettes and engine noise. He identified the aircraft as a German bomber and said they should get under the table. Grandmother said it was a different aircraft and refused. By the time the searchlight switched on, the aircraft had dropped three bombs which only just missed the farm-house. When they heard the first bomb, they all quickly got under the table.
Sinapis pubescens Linnaeus 1767
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
Sinapis
Sinapis pubescens

description: Sinapis pubescens Linnaeus, Systema Naturae, ed. 12, 2: 445; Mantissa Plantarum: 95. 1767.
"Habitat in Siciliae monte Bussambarensi. Arduin." RCN: 4866.
 Lectotype (Jafri in Ali & Jafri, Fl. Libya 23: 24. 1977): Arduino 50, Herb. Linn. No. 845.7 (LINN).
 Current name:  Sinapis pubescens  L. (Brassicaceae).
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 854, DOI: 10.5281/zenodo.291971
MOESM1 of CHRNA5 and CHRNA3 polymorphism and lung cancer susceptibility in Palestinian population
Creators: name: Ayesh, Basim
name: Al-Masri, Rami
name: Abed, Abdalla
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. List of AS-primers for each SNP.
Unification and fermion mass relations in low string scale D-brane models
Creators: name: Gioutsos, D. V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this talk, gauge coupling evolution is analyzed in D-brane inspired models with two Higgs doublets and a U(3)xU(2)xU(1)^N gauge symmetry. In particular, we focus on D-brane configurations with two or three abelian factors. We find that the correct hypercharge assignment of the Standard Model particles is reproduced for six viable models distinguished by different brane configurations. We also investigate the bottom tau quark mass relation and find that the correct low energy m_b / m_τratio is obtained for equal b-τYukawa couplings at a string scale around 10^3 TeV.
description: 10 pages, 3 figures. Talk presented at the ``Corfu Summer Institute'', Corfu-Greece, September 4-14, 2005. To appear in the proceedings of RTN workshop on the Quest for Unification Theory Confronts Experiment
Parameterized complexity of machine scheduling: 15 open problems
Creators: name: Mnich, Matthias
name: van Bevern, René
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optimization and Control (math.OC)
subject: Computational Complexity (cs.CC)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: F.2.2; G.2.1
subject: 90B35

description: Machine scheduling problems are a long-time key domain of algorithms and complexity research. A novel approach to machine scheduling problems are fixed-parameter algorithms. To stimulate this thriving research direction, we propose 15 open questions in this area whose resolution we expect to lead to the discovery of new approaches and techniques both in scheduling and parameterized complexity theory.
description: Version accepted to Computers & Operations Research
Generalized form factors, generalized parton distributions and the spin contents of the nucleon
Creators: name: Wakamatsu, M.
name: Nakakoji, Y.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: With a special intention of clarifying the underlying spin contents of the nucleon, we investigate the generalized form factors of the nucleon, which are defined as the $n$-th $x$-moments of the generalized parton distribution functions, within the framework of the chiral quark soliton model. A particular emphasis is put on the pion mass dependence of final predictions, which we shall compare with the predictions of lattice QCD simulations carried out in the so-called heavy pion region around $m_π\simeq (700 \sim 900) {MeV}$. We find that some observables are very sensitive to the variation of the pion mass. It will be argued that the negligible importance of the quark orbital angular momentum indicated by the LHPC and QCDSF lattice collaborations might be true in the unrealistic heavy pion world, but it is not necessarily the case in our real world close to the chiral limit.
description: Final version accepted for publication in Phys. Rev. D
Sisymbrium austriacum subsp. chrysanthemum Rouy & Foucaud
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
Sisymbrium
Sisymbrium austriacum
Sisymbrium austriacum jacq. subsp. chrysanthemum (jord.) rouy & foucaud

description: Sinapis pyrenaica Linnaeus, Species Plantarum, ed. 2, 2: 934. 1763.
"Habitat in Pyrenaeis. D. Monnier." RCN: 4865.
 Lectotype (Pujadas Salvà in Cafferty & Jarvis in Taxon 51: 535. 2002): Herb. Linn. No. 845.5 (LINN).
 Current name:  Sisymbrium austriacum  Jacq. subsp.  chrysanthemum  (Jord.) Rouy & Foucaud (Brassicaceae).
 Note: The epithet “pyrenaica” is pre-occupied in Sisymbrium by Sisymbrium pyrenaica Loefl. (1758), preventing the transfer of Sinapis pyrenaica to that genus.
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 854, DOI: 10.5281/zenodo.291971
MOESM6 of PfCap380 as a marker for Plasmodium falciparum oocyst development in vivo and in vitro
Creators: name: Itsara, Leslie
name: Yaxian Zhou
name: Do, Julie
name: Samrita Dungel
name: Fishbaugher, Matthew
name: Betz, Will
name: Nguyen, Thao
name: Navarro, Mary
name: Flannery, Erika
name: Vaughan, Ashley
name: Kappe, Stefan
name: Ghosh, Anil
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 6: Figure S6. Oocyst DNA increases after six days of in vitro culture. After two, three, and six days in culture, oocysts were collected and DNA content was measured using a fluorescent nucleic acid stain specific for double-stranded DNA (dsDNA). dsDNA concentration was calculated by comparison to standards with known DNA concentrations. Mean values are shown for oocysts on days 2, 3 and 6. To determine the significance between groups, a One-way ANOVA and Tukeyâ s Test was performed. For significance, * = p < 0.05, ** = p < 0.01. The experiment was performed in triplicate, and error bars represent standard deviation.
Tentative detection of the gravitational magnification of type Ia supernovae
Creators: name: Jonsson, Jakob
name: Dahlen, Tomas
name: Goobar, Ariel
name: Mortsell, Edvard
name: Riess, Adam
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The flux from distant type Ia supernovae (SN) is likely to be amplified or de-amplified by gravitational lensing due to matter distributions along the line-of-sight. A gravitationally lensed SN would appear brighter or fainter than the average SN at a particular redshift. We estimate the magnification of 26 SNe in the GOODS fields and search for a correlation with the residual magnitudes of the SNe. The residual magnitude, i.e. the difference between observed and average magnitude predicted by the "concordance model" of the Universe, indicates the deviation in flux from the average SN. The linear correlation coefficient for this sample is r=0.29. For a similar, but uncorrelated sample, the probability of obtaining a correlation coefficient equal to or higher than this value is ~10%, i.e. a tentative detection of lensing at ~90% confidence level. Although the evidence for a correlation is weak, our result is in accordance with what could be expected given the small size of the sample.
description: 7 pages, 2 figures
Classifying Fano Complexity-One $T$-Varieties via Divisorial Polytopes
Creators: name: Ilten, Nathan
name: Mishna, Marni
name: Trainor, Charlotte
Publisher: name: arXiv
Year: 2017
Subjects: subject: Algebraic Geometry (math.AG)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: The correspondence between Gorenstein Fano toric varieties and reflexive polytopes has been generalized by Ilten and Süß to a correspondence between Gorenstein Fano complexity-one $T$-varieties and Fano divisorial polytopes. Motivated by the finiteness of reflexive polytopes in fixed dimension, we show that over a fixed base polytope, there are only finitely many Fano divisorial polytopes, up to equivalence. We classify two-dimensional Fano divisorial polytopes, recovering Huggenberger's classification of Gorenstein del Pezzo $\mathbb{K}^*$-surfaces. Furthermore, we show that any three-dimensional Fano divisorial polytope is equivalent to one involving only eight functions.
description: 18 pages, 8 figures; minor revisions