cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Moenchia erecta G. Gaertn.
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
Caryophyllales
Caryophyllaceae
Moenchia
Moenchia erecta

description: Sagina erecta Linnaeus, Species Plantarum 1: 128. 1753.
"Habitat in Galliae, Angliae, Germaniae, sterilibus glareosis." RCN: 1049.
 Lectotype (Strid in Cafferty & Jarvis in Taxon 53: 1053. 2004): Herb. Linn. No. 177.3 (LINN).
 Current name:  Moenchia erecta  (L.) G. Gaertn. & al. (Caryophyllaceae).
 Note: Williams (in J. Bot. 39: 365-369. 1901) provides a detailed historical review, noting the literature cited by Linnaeus.
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 806, DOI: 10.5281/zenodo.291971
The 1 um discontinuity in the Extragalactic Background Light spectrum: an artefact of foreground subtraction
Creators: name: Mattila, K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Several recent papers claim the detection of a near infrared Extragalactic Background Light (EBL) intensity at 1.25 - 4 um that exceeds the integrated light of galaxies by factors of >3. When combined with a claimed optical detection of the EBL at 0.80 um the EBL excess emission spectrum has a discontinuity at ~1 um. This discontinuity has given rise to an interpretation in terms of ultraviolet radiation emanating from the first generation of massive stars at redshifts of 7 - 20 (so called Population III stars). The interpretation of the NIR excess emission as being of extragalactic origin depends crucially on the model used in the subtraction of the Zodiacal Light, the dominant foreground contaminant. We estimate the Zodiacal Light at 0.80 um using on the one hand the measurement by Bernstein et al.,2002, ApJ, 571,85), with corrections for some omitted effects of atmospheric scattering and calibration, and on the other hand the model of Kelsall et al.,1998, ApJ, 508,44). There is in neither case any evidence for a step in the EBL at ~1 um. We emphasize that in order to avoid systematic effects it is essential to use the same Zodiacal Light model (Kelsall et al. 1998) for both the NIR (1.25 - 4 um) and optical (0.80 um) data. We emphasize, however, that our analysis does not allow a statement on the overall level of the NIR EBL. The contribution of the Diffuse Galactic Light to the ``EBL excess'' emission is estimated. It is found to be significant at 3 - 4 um and should be carefully evaluated in future measurements which aim at detecting an EBL signal at the level of ~10 nW m^-2 sr^-1, i.e. at the level of the integrated light of (known) galaxies.
description: 7 pages, 1 figure, accepted for publication in MNRAS
MOESM2 of Natural selection and genetic diversity of domain I of Plasmodium falciparum apical membrane antigen-1 on Bioko Island
Creators: name: Wang, Ya-Nan
name: Lin, Min
name: Liang, Xue-Yan
name: Chen, Jiang-Tao
name: Xie, Dong-De
name: Wang, Yu-Ling
name: Ehapo, Carlos
name: Eyi, Urbano
name: Huang, Hui-Ying
name: Wu, Jing-Li
name: Xu, Dan-Yan
name: Chen, Zhi-Mao
name: Cao, Yi-Long
name: Chen, Hai-Bin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 2: Recombination events in global PfAMA-1 genes. Linkage disequilibrium (LD) plots showed a non-random association between nucleotide variants in DI of PfAMA-1 at different polymorphic sites. R2 values were plotted against nucleotide distance using a two-tailed Fisherâ s exact test for statistical significance.
"The universal meaning of the quantum of action", by Jun Ishiwara
Creators: name: Pelogia, Karla
name: Brasil, Carlos Alexandre
Publisher: name: arXiv
Year: 2017
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Commented translation of the paper "Universelle Bedeutung des Wirkungsquantums", published by Jun Ishiwara in German in the Proceedings of Tokyo Mathematico-Physical Society 8 106-116 (1915). In his work, Ishiwara, tenured at Sendai University, Japan, proposed - simultaneously with Arnold Sommerfeld, William Wilson and Niels Bohr in Europe - the pase-space-integral quantization, a rule that would be incorporated into the old-quantum-mechanics formalism.
description: 11 pages, 1 figure
title: Dossiers documentaires de Bouvard et Pécuchet. Recueil g226, volume 7
Creators: name: Flaubert, Gustave
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022

description: Descriptif matériel du dossier préparatoire selon le catalogue de la Bibliothèque municipale de Rouen : "XIXe s. Papier. 338 folios numérotés de 1 à 338. Cartonné, dos toile noire",
et de son contenu, avec des compléments donnés entre crochets droits :
 F. 1. Titre : Rococo. 
F.2 -16. Temples de style rococo ; 
F. 17-21. Spécimen de divers types littéraires : style Empire ; ineptie s; littérature politique ; 
F. 22-23. Haine des romans ; 
F. 24. Titre : Sciences - Médecine - Hygiène ; 
F. 25-26. Liste de 52 ouvrages relatifs aux questions ci-dessus ; 
F. 27-137. Notes sur 54 ouvrages consultés ; 
F. 138-146. Résumé des notes sur la médecine, hygiène ; 
F. 147-148. Références bibliographiques ; 
F. 149-158. Divers : notes de lectures ; exemples de curiosités médicales ; littérature médicale ; 
F. 159-177. Œuvres posthumes du Dr Charles Lefèvre publiées par Lefèvre-Deumier ; 
F. 178. Blanc ; 
F. 179. Titre : Socialisme ; 
F. 180. Liste de 25 ouvrages traitant du sujet ci-dessus ; 
F. 181-248. Notes sur les ouvrages ci-dessus ; 
F. 249. Titre : Socialisme ; 
F. 250-267. Résumé des notes de lectures ; 
F. 268. Liste de 10 ouvrages relatifs au socialisme ; 
F. 269-283. Notes sur les ouvrages portés sur la liste ci-dessus ; 
F. 284. Titre : Papiers trouvés çà et là sur la table de travail ; 
F. 285-290. Pièces diverses : Rapport sur l’état sanitaire de Jumièges et ses environs ; références bibliographiques ; annonce en Librairie de Madame Bovary, Salammbô, etc. ; 
F. 291. Titre : À classer ; 
F. 292-316. Pièces diverses : références sur personnages et mœurs de l'Antiquité ; sur la topographie du bocage normand ; Dictionnaire des Turfistes ; notes sur La police dévoilée… par Fromentin ; Leçons de Michelet, 1847-48 ; L'Époque sans nom : Esquisses de Paris, 1830-33 par A. Bazin ; Mémoires de Billard de Veaux ; La France en 1829 et 1830 par Lady Morgan ; etc. ; 
F. 317-338. Notes et références sur la question de l’éducation [chapitre X de Bouvard et Pécuchet] et pièces diverses.
Hydrodynamical constraints on bubble wall velocity
Creators: name: Krajewski, Tomasz
name: Lewicki, Marek
name: Zych, Mateusz
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Terminal velocity reached by bubble walls in first order phase transitions is an important parameter determining both primordial gravitational-wave spectrum and production of baryon asymmetry in models of electroweak baryogenesis. We developed a numerical code to study the real-time evolution of expanding bubbles and investigate how their walls reach stationary states. Our results agree with profiles obtained within the so-called bag model with very good accuracy, however, not all such solutions are stable and realised in dynamical systems. Depending on the exact shape of the potential there is always a range of wall velocities where no steady state solutions exist. This behaviour in deflagrations was explained by hydrodynamical obstruction where solutions that would heat the plasma outside the wall above the critical temperature and cause local symmetry restoration are forbidden. For even more affected hybrid solutions causes are less straight forward, however, we provide a simple numerical fit allowing one to verify if a solution with a given velocity is allowed simply by computing the ratio of the nucleation temperature to the critical one for the potential in question.
description: 11 pages, 7 figures, version published in PRD
Reconstructing the Cosmic Expansion History with a Monotonicity Prior
Creators: name: Xu, Youhua
name: Zhan, Hu
name: Cheung, Yeuk-Kwan Edna
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The cosmic expansion history, mapped by the Hubble parameter as a function of redshift, offers the most direct probe of the dark energy equation of state. One way to determine the Hubble parameter at different redshifts is essentially differentiating the cosmic age or distance with respect to redshift, which may incur large numerical errors with observational data. Taking the scenario that the Hubble parameter increases monotonically with redshift as a reasonable prior, we propose to enforce the monotonicity when reconstructing the Hubble parameter at a series of redshifts. Tests with mock type Ia supernova (SN Ia) data show that the monotonicity prior does not introduce significant biases and that errors on the Hubble parameter are greatly reduced compared to those determined with a flat prior at each redshift. Results from real SN Ia data are in good agreement with those based on ages of passively evolving galaxies. Although the Hubble parameter reconstructed from SN Ia distances does not necessarily provide more information than the distances themselves do, it offers a convenient way to compare with constraints from other methods. Moreover, the monotonicity prior is expected to be helpful to other probes that measure the Hubble parameter at multiple redshifts (e.g., baryon acoustic oscillations), and it may be generalized to other cosmological quantities that are reasonably monotonic with redshift.
description: 10 pages, 7 figures, 3 tables; v3 added Monte Carlo analysis results; accepted for publication
Neutrinoless Double Beta Decay and Future Neutrino Oscillation Precision Experiments
Creators: name: Choubey, S.
name: Rodejohann, W.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We discuss to what extent future precision measurements of neutrino mixing observables will influence the information we can draw from a measurement of (or an improved limit on) neutrinoless double beta decay. Whereas the Delta m^2 corresponding to solar and atmospheric neutrino oscillations are expected to be known with good precision, the parameter theta_{12} will govern large part of the uncertainty. We focus in particular on the possibility of distinguishing the neutrino mass hierarchies and on setting a limit on the neutrino mass. We give the largest allowed values of the neutrino masses which allow to distinguish the normal from the inverted hierarchy. All aspects are discussed as a function of the uncertainty stemming from the involved nuclear matrix elements. The implications of a vanishing, or extremely small, effective mass are also investigated. By giving a large list of possible neutrino mass matrices and their predictions for the observables, we finally explore how a measurement of (or an improved limit on) neutrinoless double beta decay can help to identify the neutrino mass matrix if more precise values of the relevant parameters are known.
description: 35 pages, 12 figures. Comments and references added. To appear in PRD
Plateau de Bure Interferometer Observations of the Disk and Outflow of HH30
Creators: name: Pety, Jérôme
name: Gueth, Frédéric
name: Guilloteau, Stéphane
name: Dutrey, Anne
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: HH30 is a well-known Pre-Main-Sequence star in Taurus. HST observations have revealed a flared, edge-on disk driving a highly-collimated optical jet, making this object a case study for the disk-jet-outflow paradigm. We obtained high angular resolution (about 1") observations of the dust continuum at 2.7 and 1.3 mm, and of the 12CO(2-1), 13CO(2-1) & (1-0), C18O(1-0) emissions around HH30. A standard disk model is used to fit the 13CO(2-1) uv-plane visibilities and derive the disk properties, and the stellar mass. It results that HH30 is a low mass TTauri of spectral type around M1 and age 1 to 4 Myrs, surrounded by a medium size Keplerian disk, of mass around 4e-3 Msun and outer radius 420 AU. The disk rotation vector points toward the North-Eastern jet. Using a distance of 140 pc, we deduce a stellar mass of 0.45 Msun. A highly asymmetric outflow originates from the inner parts of the disk. It presents to first order a conical morphology with a 30 degree half opening angle and a constant (12 km/s) radial velocity field. Outflow rotation was searched for but not found. These observations do not enable to assign the origin of the molecular outflow to entrainment by the optical jet or to a disk wind. In the latter case, the upper limit of the outflow rotation velocity implies an origin in the inner 15 AU of the disk.
description: 20 pages, 15 PostScript figures. Accepted for publication in Astronomy & Astrophysics. Uses aa LaTeX macros
Sagina procumbens 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
Caryophyllales
Caryophyllaceae
Sagina
Sagina procumbens

description: Sagina procumbens Linnaeus, Species Plantarum 1: 128. 1753.
"Habitat in Europae pascuis sterilibus uliginosis aridis." RCN: 1047.
 Lectotype (Jonsell & Jarvis in Jarvis & al., Regnum Veg. 127: 83. 1993): [icon] "Alsine pusilla graminea, flore tetrapetalo" in Séguier, Pl. Veron. 1:421,417, t. 5, f. 3. 1745.
 Generitype of Sagina Linnaeus (vide Hitchcock, Prop. Brit. Bot.: 127. 1929).
 Current name:  Sagina procumbens  L. (Caryophyllaceae).
 Note: Jonsell & Jarvis (in Nordic J. Bot. 14: 158. 1994) provided an explanation of their formal 1993 typification.
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 806, DOI: 10.5281/zenodo.291971
Distinct roles of GABAergic interneurons in the regulation of striatal output pathways.
Creators: name: Aryn Gittis
name: Nelson, Alexandra B.
name: Myo T. Thwin
name: Palop, Jorge J.
name: Kreitzer, Anatol C.
Publisher: name: Carnegie Mellon University
Year: 2010
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Striatal GABAergic microcircuits are critical for motor function, yet their properties remain enigmatic due to difficulties in targeting striatal interneurons for electrophysiological analysis. Here, we use Lhx6-GFP transgenic mice to identify GABAergic interneurons and investigate their regulation of striatal direct- and indirect-pathway medium spiny neurons (MSNs). We find that the two major interneuron populations, persistent low-threshold spiking (PLTS) and fast spiking (FS) interneurons, differ substantially in their excitatory inputs and inhibitory outputs. Excitatory synaptic currents recorded from PLTS interneurons are characterized by a small, nonrectifying AMPA receptor-mediated component and a NMDA receptor-mediated component. In contrast, glutamatergic synaptic currents in FS interneurons have a large, strongly rectifying AMPA receptor-mediated component, but no detectable NMDA receptor-mediated responses. Consistent with their axonal morphology, the output of individual PLTS interneurons is relatively weak and sparse, whereas FS interneurons are robustly connected to MSNs and other FS interneurons and appear to mediate the bulk of feedforward inhibition. Synaptic depression of FS outputs is relatively insensitive to firing frequency, and dynamic-clamp experiments reveal that these short-term dynamics enable feedforward inhibition to remain efficacious across a broad frequency range. Surprisingly, we find that FS interneurons preferentially target direct-pathway MSNs over indirect-pathway MSNs, suggesting a potential mechanism for rapid pathway-specific regulation of striatal output pathways.
Magnetar-Powered Supernovae in Two Dimensions. II. Broad-Line Supernovae Ic
Creators: name: Chen, Ke-Jung
name: Moriya, Takashi J.
name: Woosley, Stan
name: Sukhbold, Tuguldur
name: Whalen, Daniel J.
name: Suwa, Yudai
name: Bromm, Volker
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Nascent neutron stars with millisecond periods and magnetic fields in excess of $10^{16}$ Gauss can drive highly energetic and asymmetric explosions known as magnetar-powered supernovae. These exotic explosions are one theoretical interpretation for supernovae Ic-BL which are sometimes associated with long gamma-ray bursts. Twisted magnetic field lines extract the rotational energy of the neutron star and release it as a disk wind or a jet with energies greater than 10$^{52}$ erg over $\sim 20$ sec. What fractions of the energy of the central engine go into the wind and the jet remain unclear. We have performed two-dimensional hydrodynamical simulations of magnetar-powered supernovae (SNe) driven by disk winds and jets with the CASTRO code to investigate the effect of the central engine on nucleosynthetic yields, mixing, and light curves. We find that these explosions synthesize less than 0.05 Msun of Ni and that this mass is not very sensitive to central engine type. The morphology of the explosion can provide a powerful diagnostic of the properties of the central engine. In the absence of a circumstellar medium these events are not very luminous, with peak bolometric magnitudes $M_b \sim -16.5 $ due to low Ni production.
description: Accepted to ApJ
Brief details of Great Uncle, who survived war but died soon afterwards and was posthumously awarded medals
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: Great Uncle who survived the war - but then was digging out sand to fill sand-bags when the heap collapsed on top of him and he was killed. The medals were awarded to him posthumously
Letter Regarding Memorandum of Conversation
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1967
Subjects: Box 232 Folder 13
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Letter from Read to Rostow attaching memorandum of conversation for White house approval prior to distribution.
A tin of unknown content! Needs further investigation by owner
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: A tin box had been found in the attic of house. It contained correspondence linked to the Bowerman family.
Subgroups of direct products of elementarily free groups
Creators: name: Bridson, Martin R
name: Howie, James
Publisher: name: arXiv
Year: 2005
Subjects: subject: Group Theory (math.GR)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 20F06, 20E08, 20F67, 20J05

description: We exploit Zlil Sela's description of the structure of groups having the same elementary theory as free groups: they and their finitely generated subgroups form a prescribed subclass E of the hyperbolic limit groups. We prove that if $G_1,...,G_n$ are in E then a subgroup $Γ\subset G_1\times...\times G_n$ is of type $\FP_n$ if and only if $Γ$ is itself, up to finite index, the direct product of at most $n$ groups from $\mathcal E$. This answers a question of Sela.
description: 19 pages, no figures
Telegram Regarding President Johnson's Decision
Creators: name: United States. Embassy (Belgrade)
Publisher: name: The University of Texas at Austin
Year: 1964
Subjects: Box 232 Folder 2
Box 232 Folder 02
Yugoslavia -- Politics and government -- 1945-1980
Yugoslavia -- Foreign relations -- 1945-1980 -- Soviet Union

description: Telegram detailing welcoming of President Johnson's decision to continue MFN treatment for Yugoslavia.
SceneCut: Joint Geometric and Object Segmentation for Indoor Scenes
Creators: name: Pham, Trung
name: Do, Thanh-Toan
name: Sünderhauf, Niko
name: Reid, Ian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Robotics (cs.RO)
subject: FOS: Computer and information sciences

description: This paper presents SceneCut, a novel approach to jointly discover previously unseen objects and non-object surfaces using a single RGB-D image. SceneCut's joint reasoning over scene semantics and geometry allows a robot to detect and segment object instances in complex scenes where modern deep learning-based methods either fail to separate object instances, or fail to detect objects that were not seen during training. SceneCut automatically decomposes a scene into meaningful regions which either represent objects or scene surfaces. The decomposition is qualified by an unified energy function over objectness and geometric fitting. We show how this energy function can be optimized efficiently by utilizing hierarchical segmentation trees. Moreover, we leverage a pre-trained convolutional oriented boundary network to predict accurate boundaries from images, which are used to construct high-quality region hierarchies. We evaluate SceneCut on several different indoor environments, and the results show that SceneCut significantly outperforms all the existing methods.
description: Published in ICRA 2018
Tomography of a displacement photon counter for discrimination of single-rail optical qubits
Creators: name: Izumi, Shuro
name: Neergaard-Nielsen, Jonas S.
name: Andersen, Ulrik L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate the performance of a Kennedy receiver, which is known as a beneficial tool in optical coherent communications, to the quantum state discrimination of the two superpositions of vacuum and single photon states corresponding to the $\hatσ_x$ eigenstates in the single-rail encoding of photonic qubits. We experimentally characterize the Kennedy receiver in vacuum-single photon two-dimensional space using quantum detector tomography and evaluate the achievable discrimination error probability from the reconstructed measurement operators. We furthermore derive the minimum error rate obtainable with Gaussian transformations and homodyne detection. Our proof of principle experiment shows that the Kennedy receiver can achieve a discrimination error surpassing homodyne detection.
Bartonia virginica Britton
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
Gentianales
Gentianaceae
Bartonia
Bartonia virginica

description: Sagina virginica Linnaeus, Species Plantarum 1: 128. 1753.
"Habitat in Virginia inter muscos ad margines fontium. D. Gronovius." RCN: 1050.
 Lectotype (Gillett in Rhodora 61: 44, 49. 1959): Clayton 649 (BM-000051719).
 Current name:  Bartonia virginica  (L.) Britton & al. (Gentianaceae).
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 806, DOI: 10.5281/zenodo.291971
Coupling a Detailed Transport Model to the Integrated Assessment Model REMIND
Creators: name: Rottoli, Marianna
name: Dirnaichner, Alois
name: Kyle, Page
name: Baumstark, Lavinia
name: Pietzcker, Robert
name: Luderer, Gunnar
Publisher: name: Technische Universität Berlin
Year: 2021
Subjects: subject: 300 Sozialwissenschaften::330 Wirtschaft::333 Boden- und Energiewirtschaft
subject: Integrated Assessment Model
subject: transport model
subject: models coupling
subject: alternative vehicles

description: The transport sector is a crucial bottleneck in the decarbonization challenge. To study the sector’s decarbonization potential in the wider systems perspective, we couple a large-scale integrated assessment model, Regionalized Model of INvestments and Development (REMIND), to a detailed transport model, Energy Demand Generator-Transport (EDGE-T). This approach allows the analysis of mobility futures in the context of long-term and global energy sector transformations, at a high level of modal and technological granularity and internal consistency. The runtime of the coupled system increases by ~ 15–20% compared with a REMIND standalone application, and first convergence tests are promising. To illustrate the capabilities of our modeling approach, we focus on a reference pathway for Europe. Preliminary results indicate that transport service demands grow in the next decades for both passenger and freight transport. Transport system emissions are expected to decrease in the same time range, due to a shift towards electric drivetrains, advanced vehicles, more efficient modes as well as a slight increase in the share of biofuels.
Nonlinear evolution equations in QCD and effective Hamiltonian at high energy
Creators: name: Stasto, A. M.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this talk I briefly present recent developments in the theory of the Color Glass Condensate. The duality between the dense and dilute regimes of the gluon field is discussed as well as the effective selfdual Hamiltonian which includes both Pomeron merging and Pomeron splitting.
description: 4 pages. Talk given at the DIS 2005 Workshop, Madison WI,USA, April 27 - May 1
Sagittaria lancifolia Linnaeus 1759
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Alismatales
Alismataceae
Sagittaria
Sagittaria lancifolia

description: Sagittaria lancifolia Linnaeus, Systema Naturae, ed. 10, 2: 1270. 1759.
["Habitat in America."] Sp. Pl., ed. 2, 2: 1411 (1763). RCN: 7202.
 Lectotype (Haynes & Holm-Nielsen, Fl. Neotropica 64: 89. 1994): Browne, Herb. Linn. No. 1124.6 (LINN).
 Current name:  Sagittaria lancifolia  L. (Alismataceae).
 Note: Although Bogin (in Mem. New York Bot. Gard. 9: 214. 1955) discussed the original material for this name, no type was designated.
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 pages 806-807, DOI: 10.5281/zenodo.291971
A dip in the UHECR spectrum and the transition from galactic to extragalactic cosmic rays
Creators: name: Aloisio, R.
name: Berezinsky, V.
name: Blasi, P.
name: Gazizov, A.
name: Grigorieva, S.
name: Hnatyk, B.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The dip is a feature in the diffuse spectrum of ultra-high energy (UHE) protons caused by electron-positron pair production on the cosmic microwave background (CMB) radiation. For a power-law generation spectrum $E^{-2.7}$, the calculated position and shape of the dip is confirmed with high accuracy by the spectra observed by the Akeno-AGASA, HiRes, Yakutsk and Fly's Eye detectors. When the particle energies, measured in these detectors, are calibrated by the dip, their fluxes agree with a remarkable accuracy. The predicted shape of the dip is quite robust. The dip is only modified strongly when the fraction of nuclei heavier than protons is high at injection, which imposes some restrictions on the mechanisms of acceleration operating in UHECR sources. The existence of the dip, confirmed by observations, implies that the transition from galactic to extragalactic cosmic rays occurs at $E \lsim 1\times 10^{18}$ eV. We show that at energies lower than a characteristic value $E_{\rm cr}\approx 1\times 10^{18}$ eV, the spectrum of extragalactic cosmic rays flattens in all cases of interest, and it provides a natural transition to a steeper galactic cosmic ray spectrum. This transition occurs at some energy below $E_{\rm cr}$, corresponding to the position of the so-called second knee. We discuss extensively the constraints on this model imposed by current knowledge of acceleration processes and sources of UHECR and compare it with the traditional model of transition at the ankle.
description: Version Accepted for Publication in Astroparticle Physics (minor changes)
Limnophytum obtusifolium Miq.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Alismatales
Alismataceae
Limnophytum
Limnophytum obtusifolium

description: Sagittaria obtusifolia Linnaeus, Species Plantarum 2: 993. 1753.
"Habitat in Asia." RCN: 7201.
 Lectotype (Carter in Hubbard & Milne-Redhead, Fl. Trop. E. Africa, Alismataceae: 9. 1960): [icon] "Sagittariae foliis planta glomerato fructu, monopyrene, Coriandri fere figura" in Plukenet, Phytographia: t. 220, f. 7. 1692; Almag. Bot.: 326. 1696. - Typotype: Herb. Sloane 97: 181 (BM-SL).
 Current name:  Limnophytum obtusifolium  (L.) Miq. (Alismataceae).
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 807, DOI: 10.5281/zenodo.291971
Distinct modes of regulated receptor insertion to the somatodendritic plasma membrane.
Creators: name: Yudowski, Guillermo A.
name: Manojkumar Puthenveedu
name: Zastrow, Mark Von
Publisher: name: Carnegie Mellon University
Year: 2006
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Many neural signaling receptors are regulated by endocytosis, but little is known about receptor insertion into the plasma membrane. Time-lapse imaging of the beta2 adrenergic receptor expressed in cultured rat hippocampal neurons, using pH-sensitive green fluorescent protein tagging and total internal reflection fluorescence microscopy, resolved distinct vesicular fusion events mediating receptor insertion into the somatodendritic plasma membrane. A 'transient' insertion mode resulted in rapid lateral dispersion of receptors immediately after insertion. A 'persistent' insertion mode resulted in the retention of inserted receptors in surface-accessible domains, which were relatively immobile for a prolonged 'wait' period before dispersing laterally. Distinct insertion modes were oppositely regulated by receptor activation and by mechanisms differing in their dependence on the signaling effector cyclic AMP-dependent protein kinase. These results reveal a new mechanism for homeostatic regulation of postsynaptic signaling and a 'kiss-and-wait' mode of regulated membrane protein insertion in neurons.
Microseismic source imaging using physics-informed neural networks with hard constraints
Creators: name: Huang, Xinquan
name: Alkhalifah, Tariq
Publisher: name: arXiv
Year: 2023
Subjects: subject: Geophysics (physics.geo-ph)
subject: Machine Learning (cs.LG)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Microseismic source imaging plays a significant role in passive seismic monitoring. However, such a process is prone to failure due to aliasing when dealing with sparsely measured data. Thus, we propose a direct microseismic imaging framework based on physics-informed neural networks (PINNs), which can generate focused source images, even with very sparse recordings. We use the PINNs to represent a multi-frequency wavefield and then apply inverse Fourier transform to extract the source image. To be more specific, we modify the representation of the frequency-domain wavefield to inherently satisfy the boundary conditions (the measured data on the surface) by means of a hard constraint, which helps to avoid the difficulty in balancing the data and PDE losses in PINNs. Furthermore, we propose the causality loss implementation with respect to depth to enhance the convergence of PINNs. The numerical experiments on the Overthrust model show that the method can admit reliable and accurate source imaging for single- or multiple- sources and even in passive monitoring settings. Compared with the time-reversal method, the results of the proposed method are consistent with numerical methods but less noisy. Then, we further apply our method to hydraulic fracturing monitoring field data, and demonstrate that our method can correctly image the source with fewer artifacts.
description: IEEE Transactions on Geoscience and Remote Sensing 2024
The Gravitino in Gaugino Mediation
Creators: name: Buchmueller, Wilfried
name: Hamaguchi, Koichi
name: Kersten, Joern
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show that for gaugino mediated supersymmetry breaking the gravitino mass is bounded from below. For a size of the compact dimensions of order the unification scale and a cutoff given by the higher-dimensional Planck mass, we find $m_{3/2} \gtrsim 10 GeV$. In a large domain of parameter space, the gravitino is the lightest superparticle with a scalar $\tildeτ$-lepton as the next-to-lightest superparticle.
description: 10 pages, 4 figures; v2: references added
“It's the Ride of Your Life”: A Qualitative Study on Survivor Awareness and Understanding of Blood and Marrow Transplantation
Creators: name: McErlean, Gemma
name: Ashley, C
name: Pradhan, A
name: Paterson, A
name: Farnham, G
name: Owen, F
name: Watson, AM
name: Presgrave, Peter
name: Yenson, V
name: Kerridge, I
name: Halcomb, Elizabeth
Publisher: name: University of Wollongong
Year: 2025
Subjects: classificationCode: 42
subject: Health sciences
subject: FOS: Health sciences
classificationCode: 4203
subject: Health services and systems
classificationCode: 3211
subject: Oncology and carcinogenesis
classificationCode: 4205
subject: Nursing

description: Objective: This paper describes blood and marrow transplantation (BMT) survivors’ and carers' knowledge and understanding of BMT and long-term care requirements. Methods: Semistructured, online interviews with 22 BMT survivors and 6 carers were used to collect qualitative data. Interviews were audio-recorded, transcribed verbatim, and analyzed using thematic analysis. Results: Findings indicate the diversity of information and education received by survivors, the importance of timing in the delivery of information, and the need to provide education as an ongoing intervention in the long-term care provided. Conclusions: The health, psychological, and functional status of BMT survivors is significantly improved by the provision of better education, understanding, and decision-making around their long-term care. Many survivors lack a good understanding of the BMT process, the late effects of BMT, and the need for and mechanism of long-term follow-up. As the number of BMT survivors increases over time, improvements in how and where education and support are provided need to be addressed to ensure adherence to recommended long-term follow-up requirements. Implications for Nursing Practice: Nurses who work with BMT survivors should continuously reassess survivors' knowledge and understanding of their condition and provide person-centered education and resources to assist learning and treatment adherence throughout the transplant journey. Further research is necessary to explore the validity and processes of consent for BMT and establish the best model of care for long-term follow-up and education.
X-shooter search for outgassing from Main Belt Comet P/2012 T1 (Pan-STARRS)
Creators: name: Snodgrass, Colin
name: Yang, Bin
name: Fitzsimmons, Alan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Main Belt Comets are a recently identified population of minor bodies with stable asteroid-like orbits but cometary appearances. Sublimation of water ice is the most likely mechanism for their recurrent activity (i.e. dust tails and dust comae), although there has been no direct detection of gas. These peculiar objects could hold the key to the origin of water on Earth. In this paper we present a search for the gas responsible for lifting dust from P/2012 T1 (Pan-STARRS), and review previous attempts at such measurements. To date such searches have mainly been indirect, looking for the common cometary gas CN rather than gasses related to water itself. We use the VLT and X-shooter to search for emission from OH in the UV, a direct dissociation product of water. We do not detect any emission lines, and place an upper limit on water production rate from P/2012 T1 of $8-9\times10^{25}$ molecules s$^{-1}$. This is similar to limits derived from observations using the Herschel space telescope. We conclude that the best current facilities are incapable of detecting water emission at the exceptionally low levels required to produce the observed activity in Main Belt Comets.
description: 6 pages, accepted for publication in A&A
A comparison of 7 Tesla MR spectroscopic imaging and 3 Tesla MR fingerprinting for tumor localization in glioma patients
Creators: name: Lazen, Philipp
name: Cardoso, Pedro Lima
name: Sharma, Sukrit
name: Cadrien, Cornelius
name: Roetzer-Pejrimovsky, Thomas
name: Furtner, Julia
name: Strasser, Bernhard
name: Hingerl, Lukas
name: Lipka, Alexandra
name: Preusser, Matthias
name: Marik, Wolfgang
name: Bogner, Wolfgang
name: Widhalm, Georg
name: Rössler, Karl
name: Trattnig, Siegfried
name: Hangel, Gilbert
Publisher: name: arXiv
Year: 2023
Subjects: subject: Medical Physics (physics.med-ph)
subject: FOS: Physical sciences

description: This paper investigates the correlation between magnetic resonance spectroscopic imaging (MRSI) and magnetic resonance fingerprinting (MRF) in glioma patients by comparing neuro-oncological markers obtained from MRSI to T1/T2 maps from MRF.
 Data from 12 consenting patients with gliomas were analyzed by defining hotspots for T1, T2 and various metabolic ratios, and comparing them using Sørensen-Dice Similarity Coefficients (DSCs) and the distances between their centers of intensity (COIDs).
 Median DSCs between MRF and the tumor segmentation were 0.73 (T1) and 0.79 (T2). The DSCs between MRSI and MRF were highest for Gln/tNAA (T1: 0.75, T2: 0.80, tumor: 0.78), followed by Gly/tNAA (T1: 0.57, T2: 0.62, tumor: 0.54) and tCho/tNAA (T1: 0.61, T2: 0.58, tumor: 0.45). The median values in the tumor hotspot were T1=1724 ms, T2=86 ms, Gln/tNAA=0.61, Gly/tNAA=0.28, Ins/tNAA=1.15, and tCho/tNAA=0.48, and, in the peritumoral region, were T1=1756 ms, T2=102ms, Gln/tNAA=0.38, Gly/tNAA=0.20, Ins/tNAA=1.06, and tCho/tNAA=0.38, and, in the NAWM, were T1=950 ms, T2=43 ms, Gln/tNAA=0.16, Gly/tNAA=0.07, Ins/tNAA=0.54, and tCho/tNAA=0.20.
 The results of this study constitute the first comparison of 7T MRSI and 3T MRF, showing a good correspondence between these methods.
description: Includes 3 tables, 6 figures, 3 supplementary tables, and 4 supplementary figures
title: Avant-propos_Manuel spécial pour l'élevage du lapin-bélier
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Avant-propos
description: ID_PARA_00626
Effect of motions in prominences on the helium resonance lines in the extreme ultraviolet
Creators: name: Labrosse, Nicolas
name: Gouttebroze, Pierre
name: Vial, Jean-Claude
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We aim at studying the effect of radial motions on the spectrum emitted by moving prominences in the helium resonance lines and at facilitating the interpretation of observations, in order to improve our understanding of these dynamic structures. We develop our non-local thermodynamic equilibrium radiative transfer code formerly used for the study of quiescent prominences. The new numerical code is now able to solve the statistical equilibrium and radiative transfer equations in the non-static case by using velocity-dependent boundary conditions for the solution of the radiative transfer problem. This first study investigates the effects of different physical conditions (temperature, pressure, geometrical thickness) on the emergent helium radiation. The motion of the prominence plasma induces a Doppler dimming effect on the resonance lines of He I and He II. The velocity effects are particularly important for the He II 304 A line as it is mostly formed by resonant diffusion of incident radiation under prominence conditions. The He I resonance lines at 584 and 537 A also show some sensitivity to the motion of the plasma, all the more when thermal emission is not too important in these lines. We also show that it is necessary to consider partial redistribution in frequency for the scattering of the incident radiation. This set of helium lines offers strong diagnostic possibilities that can be exploited with the SOHO spectrometers and with the EIS spectrometer on board the Hinode satellite. The addition of other helium lines and of lines from other elements (in particular hydrogen) in the diagnostics will further enhance the strength of the method.
description: Replaced by revised version: 13 pages, 14 figures, accepted for publication in A&A
Private F L B Whitehead
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: The contributor's father was member of the 43rd Mobile Field Bakery, RASC in 1944.
Dissecting Drosophila embryonic brain development using photoactivated gene expression.
Creators: name: Robertson, Katherine
name: Mergliano, Jaime
name: Minden, Jonathan
Publisher: name: Carnegie Mellon University
Year: 2003
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: The Drosophila brain is generated by a complex series of morphogenetic movements. To better understand brain development and to provide a guide for experimental manipulation of brain progenitors, we created a fate map using photoactivated gene expression to mark cells originating within specific mitotic domains and time-lapse microscopy to dynamically monitor their progeny. We show that mitotic domains 1, 5, and 9 give rise to discrete cell populations within specific regions of the brain. Two novel observations were that the antennal sensory system, composed of four disparate cell clusters, arose from mitotic domain 5 and that mitotic domain B produced glial cells, while neurons were produced from mitotic domains 1, 5, and 9. Time-lapse analysis of marked cells showed complex mitotic and migratory patterns for cells derived from these mitotic domains. Photoactivated gene expression was also used either to kill, to induce ectopic divisions, or to alter cell fate. This revealed that deficits were not repopulated, while ectopic cells were removed and extra glia were tolerated.
Sagittaria lancifolia Linnaeus 1759
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Alismatales
Alismataceae
Sagittaria
Sagittaria lancifolia

description: Sagittaria pugioniformis Linnaeus, Plantae Surinamenses: 15. 1775.
"Habitat [in Surinamo.]" RCN: 7204.
 Lectotype (Haynes & Holm-Nielsen, Fl. Neotropica 64: 90. 1994): Herb. Linn. No. 1124.7 (LINN).
 Current name:  Sagittaria lancifolia  L. (Alismataceae).
 Note: Although Bogin (in Mem. New York Bot. Gard. 9: 191. 1955) referred to "the Linnaean type specimen", he did not indicate what he believed it to be.
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 807, DOI: 10.5281/zenodo.291971
Theory of a Quantum Scanning Microscope for Cold Atoms
Creators: name: Yang, Dayou
name: Laflamme, Catherine
name: Vasilyev, Denis
name: Baranov, Mikhail
name: Zoller, Peter
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We propose and analyze a scanning microscope to monitor `live' the quantum dynamics of cold atoms in a Cavity QED setup. The microscope measures the atomic density with subwavelength resolution via dispersive couplings to a cavity and homodyne detection within the framework of continuous measurement theory. We analyze two modes of operation. First, for a fixed focal point the microscope records the wave packet dynamics of atoms with time resolution set by the cavity lifetime. Second, a spatial scan of the microscope acts to map out the spatial density of stationary quantum states. Remarkably, in the latter case, for a good cavity limit, the microscope becomes an effective quantum non-demolition (QND) device, such that the spatial distribution of motional eigenstates can be measured back-action free in single scans, as an emergent QND measurement.
description: 4+5 pages, 4+1 figures; published version