cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Cell micromanipulation with an active handheld micromanipulator.
Creators: name: Tabares, Jaime Cuevas
name: MacLachlan, Robert
name: Ettensohn, Charles A.
name: Riviere, Cameron N.
Publisher: name: Carnegie Mellon University
Year: 2010
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: The paper describes the use of an active handheld micromanipulator, known as Micron, for micromanipulation of cells. The device enables users to manipulate objects on the order of tens of microns in size, with the natural ease of use of a fully handheld tool. Micron senses its own position using a purpose-built microscale optical tracker, estimates the erroneous or undesired component of hand motion, and actively corrects it by deflecting its own tool tip using piezoelectric actuators. Benchtop experiments in tip positioning show that active compensation can reduce positioning error by up to 51% compared to unaided performance. Preliminary experiments in bisection of sea urchin embryos exhibit an increased success rate when performed with the help of Micron.
Suaeda vera J. F. Gmel.
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
Amaranthaceae
Suaeda
Suaeda vera

description: Salsola fruticosa (Linnaeus) Linnaeus, Species Plantarum, ed. 2, 1: 324. 1762.
"Habitat in maritimis Galliae, Hispaniae, Persiae." RCN: 1830.
 Basionym: Chenopodium fruticosum L. (1753).
 Lectotype (Heath in Calyx 2: 78. 1992): [icon] " Sedum minus arborescens " in Munting, Naauwk. Beschryv. Aardgew.: 469, t. 469. 1696.
 Current name:  Suaeda vera  Forssk. ex J.F. Gmel. (Chenopodiaceae).
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 810, DOI: 10.5281/zenodo.291971
Neutral Higgs bosons in the SU(3)$_{L}\otimesU(1)_{N}$ model
Creators: name: Montalvo, J. E. Cieza
name: Tonasse, M. D.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The SU(3)$_L\otimesU(1)_N$ electroweak model predicts new Higgs bosons beyond the one of the standard model. In this work we investigate the signature and production of neutral SU(3)$_L\otimesU(1)_N$ Higgs bosons in the $e^-e^+$ Next Linear Collider (NLC) and in the CERN Linear Collider (CLIC). We compute the branching ratios of two of the SU(3)$_L\otimesU(1)_N$ neutral Higgs bosons and study the possibility to detect them and the $Z^\prime$ extra neutral boson of the model.
description: 17 pages, 10 figures, RevTex4
Elementary excitations in homogeneous superfluid neutron star matter: role of the neutron-proton coupling
Creators: name: Baldo, Marcello
name: Ducoin, Camille
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The thermal evolution of Neutron Stars is affected by the elementary excitations that characterize the stellar matter. In particular, the low-energy excitations, with a spectrum linear in momentum, can play a major role in the emission and propagation of neutrinos. In this paper, we focus on the elementary modes in the region of proton superfluidity, where the neutron component is expected to have a very small or zero pairing gap. We study the overall spectral functions of protons, neutrons and electrons on the basis of the Coulomb and nuclear interactions. This study is performed in the framework of the Random Phase Approximation, generalized in order to describe the response of a superfluid system. The formalism we use ensures that the Generalized Ward's Identities are satisfied. Despite their relative small fraction, the protons turn out to modify the neutron spectral function as a consequence of the nuclear neutron-proton interaction. This effect is particularly evident at the lower density, just below the crust for a density close to the saturation value, while at increasing density the neutrons and the protons are mainly decoupled. The proton spectral function is characterized by a pseudo-Goldstone mode below $ 2Δ$, twice the pairing gap, and a pair-breaking mode above $ 2Δ$. The latter merges in the sound mode of the normal phase at higher momenta. The neutron spectral function develops a collective sound mode only at the higher density. The electrons have a strong screening effect on the proton-proton interaction at the lower momenta, and decouple from the protons at higher momenta.
description: 6 figures, to appear in Phys. Rev. C
A Spectroscopic Study of Field and Runaway OB Stars
Creators: name: McSwain, M. Virginia
name: Boyajian, Tabetha S.
name: Grundstrom, Erika D.
name: Gies, Douglas R.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Identifying binaries among runaway O- and B-type stars offers valuable insight into the evolution of open clusters and close binary stars. Here we present a spectroscopic investigation of 12 known or suspected binaries among field and runaway OB stars. We find new orbital solutions for five single-lined spectroscopic binaries (HD 1976, HD 14633, HD 15137, HD 37737, and HD 52533), and we classify two stars thought to be binaries (HD 30614 and HD 188001) as single stars. In addition, we reinvestigate their runaway status using our new radial velocity data with the UCAC2 proper motion catalogs. Seven stars in our study appear to have been ejected from their birthplaces, and at least three of these runaways are spectroscopic binaries and are of great interest for future study.
description: 21 pages, 1 figure, 7 tables; Accepted to ApJ
Cell cycle dependence of protein subcellular location inferred from static, asynchronous images.
Creators: name: Taraz E. Buck
name: Rao, Arvind
name: Coelho, Luis Pedro
name: Fuhrman, Margaret H.
name: Jarvik, Jonathan
name: Berget, Peter B.
name: Murphy, Robert
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Protein subcellular location is one of the most important determinants of protein function during cellular processes. Changes in protein behavior during the cell cycle are expected to be involved in cellular reprogramming during disease and development, and there is therefore a critical need to understand cell-cycle dependent variation in protein localization which may be related to aberrant pathway activity. With this goal, it would be useful to have an automated method that can be applied on a proteomic scale to identify candidate proteins showing cell-cycle dependent variation of location. Fluorescence microscopy, and especially automated, high-throughput microscopy, can provide images for tens of thousands of fluorescently-tagged proteins for this purpose. Previous work on analysis of cell cycle variation has traditionally relied on obtaining time-series images over an entire cell cycle; these methods are not applicable to the single time point images that are much easier to obtain on a large scale. Hence a method that can infer cell cycle-dependence of proteins from asynchronous, static cell images would be preferable. In this work, we demonstrate such a method that can associate protein pattern variation in static images with cell cycle progression. We additionally show that a one-dimensional parameterization of cell cycle progression and protein feature pattern is sufficient to infer association between localization and cell cycle.
MPEC 2025-E15 : 2025 DH25
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2025 DH25

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Small Pieces of My Father's History
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: My father was a driver in the army during WW2. I was a late baby, and neither he nor anyone else ever really spoke of his time in the service. I have the feeling it marked him - we weren't close, and he wasn't very emotionally forthcoming. I don't know who the man he was before or during the war was; I only know what it left him as.
Strange stars in $f(R,\mathcal{T})$ gravity
Creators: name: Deb, Debabrata
name: Rahaman, Farook
name: Ray, Saibal
name: Guha, B. K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this article we try to present spherically symmetric isotropic strange star model under the framework of $f(R,\mathcal{T})$ theory of gravity. To this end, we consider that the Lagrangian density is an arbitrary linear function of the Ricci scalar $R$ and the trace of the energy momentum tensor~$\mathcal{T}$ given as $f\left(R,\mathcal{T}\right)=R+2χT$. We also assume that the quark matter distribution is governed by the simplest form of the MIT bag model equation of state (EOS) as $p=\frac{1}{3}\left(ρ-4B\right)$, where $B$ is the bag constant. We have obtained an exact solution of the modified form of the the Tolman-Oppenheimer-Volkoff (TOV) equation in the framework of $f(R,\mathcal{T})$ gravity theory and studied the dependence of different physical properties, viz., total mass, radius, energy density and pressure on the chosen values of $χ$. Further, to examine physical acceptability of the proposed stellar model in detail, we conducted different tests, viz. energy conditions, modified TOV equation, mass-radius relation, causality condition etc. We have precisely explained the effects arising due to the coupling of the matter and geometry on the compact stellar system. For a chosen value of the Bag constant we have predicted numerical values of different physical parameters in tabular format for the different strange stars. It is found that as the factor $χ$ increases the strange stars shrink gradually and become less massive to turn into a more compact stellar system. The maximum mass point is well within the observational limits and hence our proposed model is suitable to explain the ultra dense compact stars. For $χ=0$ we retrieve as usual the standard results of general relativity (GR).
description: 20 pages, 9 figures, 2 tables, Major revisions
On the Unification of Gauge Symmetries in Theories with Dynamical Symmetry Breaking
Creators: name: Christensen, Neil D.
name: Shrock, Robert
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyze approaches to the partial or complete unification of gauge symmetries in theories with dynamical symmetry breaking. Several types of models are considered, including those that (i) involve sufficient unification to quantize electric charge, (ii) attempt to unify the three standard-model gauge interactions in a simple Lie group that forms a direct product with an extended technicolor group, and, most ambitiously, (iii) attempt to unify the standard-model gauge interactions with (extended) technicolor in a simple Lie group.
description: 24 pages, ReVTeX
Caught in the evolutionary act: precise cis-regulatory basis of difference in the organization of gene networks of sea stars and sea urchins.
Creators: name: Hinman, Veronica F.
name: Nguyen, Albert
name: Davidson, Eric H.
Publisher: name: Carnegie Mellon University
Year: 2007
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: The regulatory control of otxbeta1/2 in the sea urchin Strongylocentrotus purpuratus and the sea star Asterina miniata provides an exceptional opportunity to determine the genomic basis of evolutionary change in gene regulatory network (GRN) architectures. Network perturbation analyses in both taxa show that Otx regulates the transcription factors gatae and krox/blimp1 and both of these transcription factors also feed back and regulate otx. The otx gene also autoregulates. This three way interaction is an example of a GRN kernel. It has been conserved for 500 million years since these two taxa last shared a common ancestor. Amid this high level of conservation we show here one significant regulatory change. Tbrain is required for correct otxbeta1/2 expression in the sea star but not in the sea urchin. In sea urchin, tbrain is not co-expressed with otxbeta1/2 and instead has an essential role in specification of the embryonic skeleton. Tbrain in these echinoderms is thus a perfect example of an orthologous gene co-opted for entirely different developmental processes. We isolate and test the sea star otxbeta1/2 cis-regulatory module and demonstrate functional binding sites for each of the predicted inputs, including Tbrain. We compare it to the logic processing operating in the sea urchin otxbeta1/2 cis-regulatory module and present an evolutionary scenario of the change in Tbrain dependence. Finally, inter-specific gene transfer experiments confirm this scenario and demonstrate evolution occurring at the level of sequence changes to the cis-regulatory module.
Salsola kali 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
Amaranthaceae
Salsola
Salsola kali

description: Salsola kali Linnaeus, Species Plantarum 1: 222. 1753.
"Habitat in Europae litoribus maris." RCN: 1819.
 Lectotype (Jonsell & Jarvis in Nordic J. Bot. 14: 155. 1994; Rilke in Biblioth. Bot. 149: 141. 1999): Herb. Burser XVI(2): 24, right specimen (UPS). - Epitype (Rilke in Biblioth. Bot. 149: 141. 1999): Herb. Clifford: 86, Salsola 2 (BM).
 Current name:  Salsola kali  L. (Chenopodiaceae).
 Note: Jonsell & Jarvis (in Nordic J. Bot. 14: 155. 1994) designated the Burser material as lectotype. However, Freitag (in litt.) has pointed out that this is a mixed sheet of S. tragus (left) and S. kali (right) and Rilke (in Biblioth. Bot. 149: 141. 1999) restricts this choice to the right-hand specimen, and also designates an epitype.
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 810, DOI: 10.5281/zenodo.291971
Lensing of 21cm Absorption "Halos" of $z\sim$20-30 First Galaxies
Creators: name: Zhang, Pengjie
name: Zheng, Zheng
name: Cen, Renyue
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Extended 21cm absorption regions (dubbed ``21cm absorption halos'') around first galaxies at $z\sim 30$ are likely the first distinctive structures accessible to radio observations. Though the radio array capable of detecting and resolving them must have $\sim 200$ km$^2$ total collecting area, given the great impact of such detections to the understanding of the reionization process and cosmology, such radio survey would be extremely profitable. As an example, we point out a potentially useful byproduct of such survey. The resolved 21cm absorption ``halos'', likely close to spherical, can serve as (almost) ideal sources for measuring the {\it cosmic shear} and mapping the matter distribution to $z\sim 30$. We investigate the expected lensing signal and consider a variety of noise contributions on the shear measurement. We find that S/N $\sim 1$ can be achieved for individual ``halos''. Given millions of 21cm absorption ``halos'' across the sky, the total S/N will be comparable to traditional shear measurement of $\sim$$10^9$ galaxies at $z\sim 1$.
description: Minor revisions and expanded discussions. Accepted to MNRAS
Impact of a star formation efficiency profile on the evolution of open clusters
Creators: name: Shukirgaliyev, Bekdaulet
name: Parmentier, Genevieve
name: Berczik, Peter
name: Just, Andreas
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study the effect of the instantaneous gas expulsion on star clusters wherein the residual gas has a density profile shallower than that of the embedded cluster. This is expected if star formation proceeds with a given SFE per free-fall time in a centrally-concentrated molecular clump. We perform direct N-body simulations whose initial conditions are generated by the program "mkhalo" "falcON" adapted for our models. Our model clusters initially have a Plummer profile and are in virial equilibrium with the gravitational potential of the cluster-forming clump. The residual gas contribution is computed based on the model of Parmentier&Pfalzner(2013). Our simulations include mass loss by stellar evolution and the tidal field of the Galaxy. We find that a star cluster with a minimum global SFE of 15% is able to survive instantaneous gas expulsion and to produce a bound cluster. Its violent relaxation lasts no longer than 20 Myr, independently of its global SFE and initial stellar mass. At the end of violent relaxation the bound fractions of surviving clusters with the same global SFEs are similar regardless of their initial stellar mass. Their subsequent lifetime in the gravitational field of the Galaxy depends on their bound stellar masses. We therefore conclude that the critical SFE needed to produce a bound cluster is 15%, which is twice smaller than earlier estimates of 33%. Thus we have improved the survival likelihood of young clusters after instantaneous gas expulsion. Those can now survive instantaneous gas expulsion with global SFEs as low as those observed for embedded clusters of Solar Neighbourhood (15-30%). This is the consequence of the star cluster having a density profile steeper than that of the residual gas. However, in terms of the effective SFE, measured by the virial ratio of the cluster at gas expulsion, our results are in agreement with previous studies.
description: Accepted for publication in Astronomy&Astrophysics, 13 pages, 10 figures
Sphalerons in the NMSSM
Creators: name: Funakubo, Koichi
name: Kakuto, Akira
name: Tao, Shuichiro
name: Toyoda, Fumihiko
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study sphaleron solutions in the next-to-minimal supersymmetric standard model. We find that the boundary condition on the singlet field at the origin of the radial coordinate is of Neumann type, while the other boundary conditions are of Dirichlet type. The sphaleron energy takes almost the same value as in the MSSM for wide range of parameters, in spite of the negative contribution from the cubic term in the Higgs potential.
description: 15 pages, 4 figures
Die Zerstörung Magdeburgs 1631
Creators: name: Tullner, Mathias
Publisher: name: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik
Year: 2018

description: Der Autor befasst sich mit den tiefen Brüchen und Kontinua in der 1.200-jährigen Geschichte der Stadt Magdeburg. Hierbei legt er den Fokus zunächst auf die fast vollständige Einäscherung dieses Zentrums des Protestantismus im Dreißigjährigen Krieg. Sodann thematisiert er die Entwicklung der Stadt zu einem Verwaltungszentrum unter brandenburgisch-preußischer Herrschaft – welche inspiriert von Bemerkungen Richard Wagners und Karl Leberecht Immermanns in der Weimarer Republik und in der DDR-Zeit in ein negatives Licht gerückt wurde. (Sabine Koch)
description: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik, Bd. 7 (2006): Jahrbuch 2005: Musikgeschichte im Zeichen der Reformation
Bassia muricata Asch.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Spermatopsida
Caryophyllales
Chenopodiaceae
Bassia
Bassia muricata

description: Salsola muricata Linnaeus, Systema Naturae, ed. 12, 2: 196; Mantissa Plantarum: 54. 1767.
"Habitat in Europa australi, Aegypto." RCN: 1831.
 Lectotype (Jafri & Rateeb in Jafri & El-Gadi, Fl. Libya 58: 23. 1978): Herb. Linn. No. 315.22 (LINN).
 Current name:  Bassia muricata  (L.) Asch. (Chenopodiaceae).
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 810, DOI: 10.5281/zenodo.291971
Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
Creators: name: Jones, D. O.
name: Scolnic, D. M.
name: Riess, A. G.
name: Rest, A.
name: Kirshner, R. P.
name: Berger, E.
name: Kessler, R.
name: Pan, Y. -C.
name: Foley, R. J.
name: Chornock, R.
name: Ortega, C. A.
name: Challis, P. J.
name: Burgett, W. S.
name: Chambers, K. C.
name: Draper, P. W.
name: Flewelling, H.
name: Huber, M. E.
name: Kaiser, N.
name: Kudritzki, R. -P.
name: Metcalfe, N.
name: Tonry, J.
name: Wainscoat, R. J.
name: Waters, C.
name: Gall, E. E. E.
name: Kotak, R.
name: McCrum, M.
name: Smartt, S. J.
name: Smith, K. W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use 1169 Pan-STARRS supernovae (SNe) and 195 low-$z$ ($z < 0.1$) SNe Ia to measure cosmological parameters. Though most Pan-STARRS SNe lack spectroscopic classifications, in a previous paper (I) we demonstrated that photometrically classified SNe can be used to infer unbiased cosmological parameters by using a Bayesian methodology that marginalizes over core-collapse (CC) SN contamination. Our sample contains nearly twice as many SNe as the largest previous SN Ia compilation. Combining SNe with Cosmic Microwave Background (CMB) constraints from Planck, we measure the dark energy equation of state parameter $w$ to be -0.989$\pm$0.057 (stat$+$sys). If $w$ evolves with redshift as $w(a) = w_0 + w_a(1-a)$, we find $w_0 = -0.912 \pm 0.149$ and $w_a =$ -0.513$\pm$0.826. These results are consistent with cosmological parameters from the Joint Lightcurve Analysis and the Pantheon sample. We try four different photometric classification priors for Pan-STARRS SNe and two alternate ways of modeling CC SN contamination, finding that no variant gives a $w$ differing by more than 2% from the baseline measurement. The systematic uncertainty on $w$ due to marginalizing over CC SN contamination, $σ_w^{\textrm{CC}} = 0.012$, is the third-smallest source of systematic uncertainty in this work. We find limited (1.6$σ$) evidence for evolution of the SN color-luminosity relation with redshift, a possible systematic that could constitute a significant uncertainty in future high-$z$ analyses. Our data provide one of the best current constraints on $w$, demonstrating that samples with $\sim$5% CC SN contamination can give competitive cosmological constraints when the contaminating distribution is marginalized over in a Bayesian framework.
description: Accepted by ApJ, data release at archive.stsci.edu/prepds/ps1cosmo/index.html
Die feierliche Beisetzung der Gebeine des Hl. Norbert im Jahre 1627 in Prag
Creators: name: Bužga, Jaroslav
Publisher: name: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik
Year: 2018

description: Dieser Beitrag verfolgt die Überführung der sterblichen Überreste Norberts von Xanten aus der Magdeburger Marienkirche bis zur Beisetzungszeremonie und den Jubiläumsfestlichkeiten ein Jahr später in der Klosterkirche zu Prag-Straho nach. Beide Feiern zugunsten des vom Stadtpatron Magdeburgs zum neuen Landespatron Böhmens Gewordenen hinterließen zwar keine konkret überlieferten Kompositionen, lassen aber angesichts der erklingenden Kantaten und Messen auf ein facettenreiches Musikleben in Prag schließen. (Sabine Koch)
description: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik, Bd. 7 (2006): Jahrbuch 2005: Musikgeschichte im Zeichen der Reformation
Color-charged Quark Matter in Astrophysics?
Creators: name: Qiu, Congxin
name: Xu, Renxin
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Color confinement is only a supposition, which has not been proved in QCD yet. It is proposed here that macroscopic quark gluon plasma in astrophysics could hardly maintain colorless because of causality. The authors expected that the existence of chromatic strange quark stars as well as chromatic strangelets preserved from the QCD phase transition in the early universe could be unavoidable if their colorless correspondents do exist.
description: 3 pages, 2 figures
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0267
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0267, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
Halogeton sativus Moq.
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
Amaranthaceae
Halogeton
Halogeton sativus

description: Salsola polyclonos Linnaeus, Systema Naturae, ed. 12, 2: 196; Mantissa Plantarum: 54. 1767.
"Habitat in Siciliae, Hispaniae maritimis." RCN: 1827.
 Lectotype (Castroviejo & al. in Anales Jard. Bot. Madrid 43: 478. 1987): Alströmer s.n. , Herb. Linn. No. 315.18 (LINN).
 Current name: Halogeton sativus (L.) Moq. (Chenopodiaceae).
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 810, DOI: 10.5281/zenodo.291971
Renormalization of a gapless Hartree-Fock approximation to a theory with spontaneously broken O(N)-symmetry
Creators: name: Ivanov, Yu. B.
name: Riek, F.
name: van Hees, H.
name: Knoll, J.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The renormalization of a gapless Phi-derivable Hartree--Fock approximation to the O(N)-symmetric lambda*phi^4 theory is considered in the spontaneously broken phase. This kind of approach was proposed by three of us in a previous paper in order to preserve all the desirable features of Phi-derivable Dyson-Schwinger resummation schemes (i.e., validity of conservation laws and thermodynamic consistency) while simultaneously restoring the Nambu--Goldstone theorem in the broken phase. It is shown that unlike for the conventional Hartree--Fock approximation this approach allows for a scale-independent renormalization in the vacuum. However, the scale dependence still persists at finite temperatures. Various branches of the solution are studied. The occurrence of a limiting temperature inherent in the renormalized Hartree--Fock approximation at fixed renormalization scale mu is discussed.
description: 11 pages, 14 figures / Version accepted by Phys. Rev. D: title and one reference changed
Caspase-independent cell engulfment mirrors cell death pattern in Drosophila embryos.
Creators: 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: Programmed cell death plays an essential role during Drosophila embryonic development. A stereotypic series of cellular changes occur during apoptosis, most of which are initiated by a caspase cascade that is triggered by a trio of proteins, RPR, HID and GRIM. The final step in apoptosis is engulfment of the cell corpse. To monitor cell engulfment in vivo, we developed a fluorogenic beta-galactosidase substrate that is cleaved by an endogenous, lysosomal beta-galactosidase activity. The pattern of cell engulfment in wild-type embryos correlated well with the known pattern of apoptosis. Surprisingly, the pattern of cell engulfment persisted in apoptosis-deficient embryos. We provide evidence for a caspase-independent engulfment process that affects the majority of cells expected to die in developing Drosophila embryos.
Spherical Trigonometry of the Projected Baseline Angle
Creators: name: Mathar, Richard J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The basic geometry of a stellar interferometer with two telescopes consists of a baseline vector and a direction to a star. Two derived vectors are the delay vector, and the projected baseline vector in the plane of the wavefronts of the stellar light. The manuscript deals with the trigonometry of projecting the baseline further outwards onto the celestial sphere. The position angle of the projected baseline is defined, measured in a plane tangential to the celestial sphere, tangent point at the position of the star. This angle represents two orthogonal directions on the sky, differential star positions which are aligned with or orthogonal to the gradient of the delay recorded in the u-v plane. The North Celestial Pole is chosen as the reference direction of the projected baseline angle, adapted to the common definition of the "parallactic" angle.
description: Corrected eq. (6) and definition of N after eq. (11)
Phase space methods for Majorana fermions
Creators: name: Joseph, Ria Rushin
name: Rosales-Zárate, Laura E. C.
name: Drummond, Peter D.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Fermionic phase space representations are a promising method for studying correlated fermion systems. The fermionic Q-function and P-function have been defined using Gaussian operators of fermion annihilation and creation operators. The resulting phase-space of covariance matrices belongs to the symmetry class D, one of the non-standard symmetry classes. This was originally proposed to study mesoscopic normal-metal-superconducting hybrid structures, which is the type of structure that has led to recent experimental observations of Majorana fermions. Under a unitary transformation, it is possible to express these Gaussian operators using real anti-symmetric matrices and Majorana operators, which are much simpler mathematical objects. We derive differential identities involving Majorana fermion operators and an antisymmetric matrix which are relevant to the derivation of the corresponding Fokker-Planck equations on symmetric space. These enable stochastic simulations either in real or imaginary time. This formalism has direct relevance to the study of fermionic systems in which there are Majorana type excitations, and is an alternative to using expansions involving conventional Fermi operators. The approach is illustrated by showing how a linear coupled Hamiltonian as used to study topological excitations can be transformed to Fokker-Planck and stochastic equation form, including dissipation through particle losses.
title: 02_1225
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Zur Magdeburger Gesangbuchgeschichte
Creators: name: Petzoldt, Martin
Publisher: name: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik
Year: 2018

description: Die Anfänge der Magdeburger Gesangbuchtradition stehen im Zusammenhang mit der lutherischen Reformation; kurz nacheinander erscheinen zwei niederdeutsche Gesangbücher, 1534 und 1536. Das erste steht in der Folge des Rostocker Gesangbuches von 1531 (Joachim Slüter), das sich an dem Wittenberger Gesangbuch von 1529 orientierte. Es erlebt viele Auflagen bis zum Ende des 16. Jahrhunderts. Das zweite kann sich auch auf die Wittenberger Anfänge von 1524 berufen, hat aber keine Fortsetzung gefunden. Eigenständig ist das große Werk Johann Spangenbergs, Cantiones Ecclesiasticae (1545), das Magdeburg als Druckort hat und für die Gottesdienstordnungen und Agenden lange Zeit überregionale Bedeutung hatte. Überraschend ist nach wie vor, daß es im 17. Jahrhundert nur eine einzige Gesangbuchedition gegeben haben sollte, nämlich die von 1654. Vor allem die verheerende Zerstörung Magdeburgs im Jahr 1631 müßte in der Folgezeit eine Edition hervorgebracht haben. Es ist davon aber nichts bekannt. Kenntnis haben wir von dieser Situation aus Gesangbuchvorreden von 1654 und 1719. Das weitere 18. Jahrhundert bringt entgegen der vorausliegenden Entwicklung eine völlig andere Situation: Im Jahr 1738 erscheinen gleichzeitig drei verschiedene Gesangbücher, die sich nur unwesentlich unterscheiden. Eines ist vom Geistlichen Ministerium der Stadt verantwortet worden und möchte sich in den Streit um die Frömmigkeit nicht kümmern (Vollständiges Gesangbuch), ein zweites wendet sich an die Christen des Herzogtums Magdeburg und transportiert pietistische Tendenzen (Neu-eingerichtetes Gesangbuch) und ein drittes beruft sich auf den Stadtrat Magdeburgs und die Aufsicht des Geistlichen Ministeriums (Neu-vermehrtes und verbessertes Gesangbuch). Die Vorrede enthält immerhin ein Indiz durch den Hinweis auf den Magdeburger Gesangbuch-Druckerstreit dieser Jahre. (der Autor) Quelle: Bibliographie des Musikschrifttums online
description: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik, Bd. 7 (2006): Jahrbuch 2005: Musikgeschichte im Zeichen der Reformation
Electromagnetic transition form factors of baryons in the space-like momentum region
Creators: name: Sanchis-Alepuz, Helios
name: Alkofer, Reinhard
name: Fischer, Christian S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present results from a calculation of the electromagnetic transition form factors between ground-state octet and decuplet baryons as well as the octet-only $Σ^0$ to $Λ$ transition. We work in the combined framework of Dyson-Schwinger equations and covariant Bethe-Salpeter equations with all elements, the baryon three body wave function, the quark propagators and the dressed quark-photon vertex determined from a well-established, momentum dependent approximation for the quark-gluon interaction. We discuss in particular the similarities among the different transitions as well as the differences induced by SU(3)-isospin symmetry breaking. We furthermore provide estimates for the slopes of the electric and magnetic $Σ^0$ to $Λ$ transitions at the zero photon momentum point.
description: 11 pages, 5 figures. arXiv admin note: text overlap with arXiv:1512.00833
Ein Magdeburger Schulbuch für den Musikunterricht aus dem Jahr 1624
Creators: name: Synofzik, Thomas
Publisher: name: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik
Year: 2018

description: Mit seinem musikalischen Unterrichtswerk "Tyrocinia" stellt sich Heinrich Grimm in eine Tradition von Musiklehrbüchern Magdeburger Kantoren vor ihm. Das teils in Deutsch, teils in Latein verfasste Schulbuch ist nicht vollständig überliefert, sondern muss aus späteren Neuauflagen rekonstruiert werden. Zunächst wird die Entstehungsgeschichte des Schulbuchs dargestellt, bevor der Inhalt des Werks analysiert wird. Dabei wird Grimms Schulbuch immer wieder in den Kontext zeitgenössischer Lehrwerke eingeordnet. - Musiktheoretisches Hauptstück ist eine achtseitige Abhandlung mit dem Titel "Kurtzer Unterricht / Wie ein junger Knabe zum Solmisiren leicht angeführet werden könne". Darüber hinaus enthält das Schulbuch reinen Notendruck, der in zwei Werkkomplexe gegliedert ist: eine Reihe von 118 textlosen Fugen und eine Sammlung von 32 textierten Werken, bei denen es sich teils um strenge Kanons, teils um frei imitatorische, teils auch um weitgehend homorhythmische Sätze handelt. Anhand von Beispielen werden die Besonderheiten dieser Sammlung herausgearbeitet. Dieses Schulbuch aus dem Jahr 1624 kann aufgrund derartiger kunstfertiger Übungsstücke als Magdeburger "Kunst der Fuge" gelten. Das ist vom Konzept des Schulwerks her nicht neuartig - doch von der Zahl der Beispiele her, dem Gebrauch von Gegenbewegung und der systematischen Anwendung auf Choralmelodien kann Grimms Sammlung einen besonderen Rang beanspruchen. (Beatrix Obal) Quelle: Bibliographie des Musikschrifttums online
description: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik, Bd. 7 (2006): Jahrbuch 2005: Musikgeschichte im Zeichen der Reformation
NLO-QCD Corrections to Dilepton Production in the Randall-Sundrum Model
Creators: name: Mathews, Prakash
name: Ravindran, V.
name: Sridhar, K.
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The dilepton production process at hadron colliders in the Randall-Sundrum (RS) model is studied at next-to-leading order in QCD. The NLO-QCD corrections have been computed for the virtual graviton exchange process in the RS model, in addition to the usual gamma, Z-mediated processes of standard Drell-Yan. K-factors for the cross-sections at the LHC and Tevatron for differential in the invariant mass, Q, and the rapidity, Y, of the lepton pair are presented. We find the K-factors are large over substantial regions of the phase space.
description: 24 pages, 12 figures
Salsola rosacea 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
Amaranthaceae
Salsola
Salsola rosacea

description: Salsola rosacea Linnaeus, Species Plantarum 1: 222. 1753, nom. cons.
"Habitat ad Asiae septentrionalis salinas." RCN: 1821.
 Conserved type (Rilke in Taxon 47: 165. 1998): Kazakstan. Taldy-Kurgan Distr, 9 Sep 1992, Freitag & Rilke 26208a (LE; iso- AA, B, C, K, KAS).
 Current name:  Salsola rosacea  L. (Chenopodiaceae).
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 810, DOI: 10.5281/zenodo.291971
Domain Wall Motion Driven by Laplace Pressure in CoFeB-MgO Nanodots with Perpendicular Anisotropy
Creators: name: Zhang, Yu
name: Zhang, Xueying
name: Vernier, Nicolas
name: Zhang, Zhizhong
name: Agnus, Guillaume
name: Coudevylle, Jean-Rene
name: Lin, Xiaoyang
name: Zhang, Yue
name: Zhang, You-Guang
name: Zhao, Weisheng
name: Ravelosona, Dafine
Publisher: name: arXiv
Year: 2017
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We have studied the magnetization reversal of CoFeB-MgO nanodots with perpendicular anisotropy for size ranging from w=400 nm to 1 μm. Contrary to previous experiments, the switching field distribution is shifted toward lower magnetic fields as the size of the elements is reduced with a mean switching field varying as 1/w. We show that this mechanism can be explained by the nucleation of a pinned magnetic domain wall (DW) at the edges of the nanodots where damages are introduced by the patterning process. As the surface tension (Laplace pressure) applied on the DW increases when reducing the size of the nanodots, we demonstrate that the depinning field to reverse the entire elements varies as 1/w. These results suggest that the presence of DWs has to be considered in the switching process of nanoscale elements and open a path toward scalable spintronic devices.
Über ästhetische Bildung an Magdeburger Schulen im 18. Jahrhundert
Creators: name: Förster, Uwe
Publisher: name: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik
Year: 2018

description: Die Magdeburger Domschule, das Pädagogium zu Kloster Berge und das Pädagogium am Kloster Unser Lieben Frauen waren zu Beginn des 18. Jahrhunderts durch die pietistische Erziehungslehre August Hermann Franckes geprägt. Im Fächerkanon waren etwa Religion, Logik, Ethik, Geschichte und die alten Sprachen enthalten, nicht aber eine musische oder künstlerische Ausbildung. Eine tragende Rolle von Kunst und Ästhetik für die Bildung bildete sich erst allmählich heraus, als Kunstwerke aus dem Schatten der historischen Betrachtung heraustraten. In der zweiten Jahrhunderthälfte zielte ästhetische Bildung schließlich auf die Steigerung der Empfindungsfähigkeit durch größere Klarheit und beschränkte sich deshalb nicht auf die Fächer Musik und Kunsterziehung, sondern war immanenter Bestandteil des Unterrichts. (Wendelin Bitzan) Quelle: Bibliographie des Musikschrifttums online
description: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik, Bd. 7 (2006): Jahrbuch 2005: Musikgeschichte im Zeichen der Reformation
Martin Agricola als Schulmann und Komponist
Creators: name: Brinzing, Armin
Publisher: name: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik
Year: 2018

description: Das pädagogische und kompositorische Wirken von Martin Agricola (1486-1556) ist eng mit der Magdeburger Lateinschule verbunden. Dabei bezog er in seine musiktheoretischen Schriften auch ausführliche Erörterungen zu Fragen des reformatorischen Schulwesens und zu aktuellen theologischen und religionspolitischen Fragen ein. Sowohl in seinen Texten als auch in seinen Kompositionen lassen sich deutliche Einflüsse der führenden Magdeburger Theologen dieser Zeit feststellen, mit denen er in engen Beziehungen stand: Nikolaus von Amsdorff, Matthias Flacius Illyricus und Nicolaus Glossenus. Für den schulischen Katechismusunterricht schrieb Agricola Werke im Stil der metrischen Odenkomposition. Seine anspruchsvollen lateinischen Motetten zeugen von seiner theologischen Bildung und sind von der religiösen und politischen Situation Magdeburgs geprägt. Die Motetten wurden nach Aussage der Magdeburger Schulordnung außerhalb der normalen Gottesdienste in eigens angesetzten mittäglichen Versammlungen der Schüler unter der Leitung Agricolas aufgeführt. (der Autor) Quelle: Bibliographie des Musikschrifttums online
description: Jahrbuch Ständige Konferenz Mitteldeutsche Barockmusik, Bd. 7 (2006): Jahrbuch 2005: Musikgeschichte im Zeichen der Reformation
Halogeton sativus Moq.
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
Amaranthaceae
Halogeton
Halogeton sativus

description: Salsola sativa Linnaeus, Species Plantarum, ed. 2, 1: 323. 1762.
"Habitat in Hispaniae australis maritimis." RCN: 1823.
Type not designated.
Original material: Herb. Linn. No. 315.9 (LINN); Herb. Linn. No. 315.32? (LINN); Herb. Linn. No. 315.18? (LINN).
 Current name:  Halogeton sativus  (L.) Moq. (Chenopodiaceae).
 Note: Blackwell & al. (in Sida 8: 161. 1979) referred to a specimen in LINN as the "type specimen" but did not distinguish between sheets 315.9, 315.18 and 315.32 (which are not part of a single gathering so Art. 9.15 does not apply). Castroviejo & al. (in Anales Jard. Bot. Madrid 43: 477. 1987) discussed these specimens in some detail and concluded that S. sativa was a new species based in part on S. souda Loefl. (1758), which Linnaeus cited in the protologue of S. sativa. Castroviejo & al. argue that S. souda is merely an orthographic variant of S. soda L. (1753) but that in 1762, Linnaeus recognised that Löfling’s plant was distinct from S. soda and gave it the name S. sativa. In the absence of Löfling 123 , they typified the name using Löfling’s description, though this is now contrary to Art. 9, a type being either a specimen or an illustration.
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 810, DOI: 10.5281/zenodo.291971