cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Spitzer c2d Survey of Nearby Dense Cores: I: First Direct Detection of the Embedded Source in IRAM 04191+1522
Creators: name: Dunham, M. M.
name: Evans, N. J.
name: Bourke, T. L.
name: Dullemond, C. P.
name: Young, C. H.
name: Brooke, T. Y.
name: Chapman, N.
name: Myers, P. C.
name: Porras, A.
name: Spiesman, W.
name: Teuben, P. J.
name: Wahhaj, Z.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the first detections of the Class 0 protostellar source IRAM 04191+1522 at wavelengths shortward of 60 microns with the Spitzer Space Telescope. We see extended emission in the Spitzer images that suggests the presence of an outflow cavity in the circumstellar envelope. We combine the Spitzer observations with existing data to form a complete dataset ranging from 3.6 to 1300 microns and use these data to construct radiative transfer models of the source. We conclude that the internal luminosity of IRAM 04191+1522, defined to be the sum of the luminosity from the internal sources (a star and a disk), is L_int = 0.08 +/- 0.04 L_sun, placing it among the lowest luminosity protostars known. Though it was discovered before the launch of the Spitzer Space Telescope, IRAM 04191+1522 falls within a new class of Very Low Luminosity Objects being discovered by Spitzer. Unlike the two other well-studied objects in this class, which are associated either with weak, compact outflows or no outflows at all, IRAM 04191+1522 has a well-defined molecular outflow with properties consistent with those expected based on relations derived from higher luminosity (L_int > 1 L_sun) protostars. We discuss the difficulties in understanding IRAM 04191+1522 in the context of the standard model of star formation, and suggest a possible explanation for the very low luminosity of this source.
description: Accepted for publication in the Astrophysical Journal. 39 pages, 9 figures. See http://peggysue.as.utexas.edu/SIRTF/ for high-resolution figures
Synaptic lability after experience-dependent plasticity is not mediated by calcium-permeable AMPARs.
Creators: name: Wen, Jing
name: Barth, Alison L.
Publisher: name: Carnegie Mellon University
Year: 2012
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Activity- or experience-dependent plasticity has been associated with the trafficking of calcium-permeable α-amino-3-hydroxy-5-methyl-4-isoxazolepropionic acid receptors (CP-AMPARs) in a number of experimental systems. In some cases it has been shown that CP-AMPARs are only transiently present and can be removed in an activity-dependent manner. Here we test the hypothesis that the presence of CP-AMPARs confers instability onto recently potentiated synapses. Previously we have shown that altered sensory input (single-whisker experience; SWE) strengthens layer 4-2/3 excitatory synapses in mouse primary somatosensory cortex, in part by the trafficking of CP-AMPARs. Both in vivo and in vitro, this potentiation is labile, and can be depressed by N-Methyl-D-aspartate receptor (NMDAR)-activation. In the present study, the role of CP-AMPARs in conferring this synaptic instability after in vivo potentiation was evaluated. We develop an assay to depress the strength of individual layer 4-2/3 excitatory synapses after SWE, using a strontium (Sr(++))-replaced artificial cerebrospinal fluid (ACSF) solution (Sr-depression). This method allows disambiguation of changes in quantal amplitude (a post-synaptic measure) from changes in event frequency (typically a presynaptic phenomenon). Presynaptic stimulation paired with post-synaptic depolarization in Sr(++) lead to a rapid and significant reduction in EPSC amplitude with no change in event frequency. Sr-depression at recently potentiated synapses required NMDARs, but could still occur when CP-AMPARs were not present. As a further dissociation between the presence of CP-AMPARs and Sr-depression, CP-AMPARs could be detected in some cells from control, whisker-intact animals, although Sr-depression was never observed. Taken together, our findings suggest that CP-AMPARs are neither sufficient nor necessary for synaptic depression after in vivo plasticity in somatosensory cortex. This article is part of a Special Issue entitled "Calcium permeable AMPARs in synaptic plasticity and disease."
Constraints on Born-Infeld gravity from the speed of gravitational waves after GW170817 and GRB 170817A
Creators: name: Jana, Soumya
name: Chakravarty, Girish Kumar
name: Mohanty, Subhendra
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The observations of gravitational waves from the binary neutron star merger event GW170817 and the subsequent observation of its electromagnetic counterparts from the gamma-ray burst GRB 170817A provide us a significant opportunity to study theories of gravity beyond general relativity. An important outcome of these observations is that they constrain the difference between the speed of gravity and the speed of light to less than $10^{-15}c$. Also, the time delay between the arrivals of gravitational waves at different detectors constrains the speed of gravity at the Earth to be in the range $0.55c < v_{gw} < 1.42c$. We use these results to constrain a widely studied modified theory of gravity: Eddington-inspired Born-Infeld (EiBI) gravity. We show that, in EiBI theory, the speed of gravitational waves in matter deviates from $c$. From the time delay in arrival of gravitational wave signals at Earth-based detectors, we obtain the bound on the theory parameter $κ$ as $\vertκ\vert \lesssim 10^{21}\, m^2$. Similarly, from the time delay between the signals of GW170817 and GRB 170817A, in a background Friedmann-Robertson-Walker universe, we obtain $\vert κ\vert \lesssim 10^{37}\, m^2$. Although the bounds on $κ$ are weak compared to other earlier bounds from the study of neutron stars, stellar evolution, primordial nucleosynthesis, etc., our bounds are from the direct observations and thus worth noting.
description: 5 pages. Published version
A theoretical review of heavy quarkonium inclusive decays
Creators: name: Vairo, Antonio
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this brief review, I summarize the current theoretical knowledge of heavy quarkonium inclusive decays, with emphasis on recent progress made in the framework of QCD effective field theories. In appendix, I list the imaginary parts of the matching coefficients of the dimension 6 and dimension 8 NRQCD four-fermion operators as presently known.
description: 16 pages, invited brief review for Modern Physics Letters A, few typos corrected
Spin-Kick Correlation in Neutron Stars: Alignment Conditions and Implications
Creators: name: Wang, Chen
name: Lai, Dong
name: Han, JinLin
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent observations of pulsar wind nebulae and radio polarization profiles revealed a tendency of the alignment between the spin and velocity directions in neutron stars. We study the condition for spin-kick alignment using a toy model, in which the kick consists of many off-centered, randomly-oriented thrusts. Both analytical considerations and numerical simulations indicate that spin-kick alignment cannot be easily achieved if the proto-neutron star does not possess some initial angular momentum, contrary to some previous claims. To obtain the observed spin-kick misalignment angle distribution, the initial spin period of the neutron star must be smaller than the kick timescale. Typically, an initial period of a hundred milliseconds or less is required.
description: 17 pages, 8 figures. Accepted by ApJ
A discrete event system specification (DEVS)-based model of consanguinity
Creators: name: Akhtar, Noreen
name: Niazi, Muaz A.
name: Mustafa, Farah
name: Hussain, Amir
Publisher: name: arXiv
Year: 2017
Subjects: subject: Social and Information Networks (cs.SI)
subject: Computers and Society (cs.CY)
subject: Discrete Mathematics (cs.DM)
subject: Populations and Evolution (q-bio.PE)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences
subject: I.2; I.2.0; I.6; J.4; J.3; B.1.2; C.4

description: Consanguinity or inter-cousin marriage is a phenomenon quite prevalent in certain regions around the globe. Consanguineous parents have a higher risk of having offspring with congenital disorders. It is difficult to model large scale consanguineous parental populations because of disparate cultural issues unique to regions and cultures across the globe. Although consanguinity, as a social problem has been studied previously, consanguinity from a biological perspective has yet to be modeled. Discrete Event System Specification (DEVS) formalism is a powerful modeling formalism for the study of intricate details of real-world complex systems. In this article, we develop a DEVS model to get an insight into the role of consanguineous marriages in the evolution of congenital disorders in a population. As proof-of-concept, we develop a consanguinity simulation model in Simio simulation software. Our results show the effectiveness of DEVS in the modeling of consanguinity effects in causing congenital defects.
description: 41 pages, 10 figures
LC-MS/MS data analysis with xcms
Creators: name: Rainer, Johannes
name: Witting, Michael
name: Neumann, Steffen
Publisher: name: Zenodo
Year: 2020
Subjects: mass spectrometry
LC-MS/MS
metabolomics
SWATH

description: The xcms software is a well established R package for the preprocessing of LC-MS-based untargeted metabolomics data. By extensively refactoring the package and re-using functionality and mass spectrometry (MS) data representation strategies from the MSnbase package for proteomics data analysis, xcms gained native MS/MS support. We recently added support for LC-MS/MS data in xcms: for data dependent acquisition (DDA) data, MS2 spectra can be identified and extracted for each detected chromatographic peak (chrom peak) or feature. For data independent acquisition (DIA) data such as SWATH data, xcms allows to perform chromatographic peak detection on MS2 data and reconstruct MS2 spectra. MS1 chrom peaks are matched to MS2 based on peak shape correlations. The recent changes in xcms, particularly the support for LC-MS/MS data analysis, facilitate an improved compound annotation for untargeted metabolomics experiments.
Tensor algebras of C*-correspondences and their C*-envelopes
Creators: name: Katsoulis, Elias G.
name: Kribs, David W.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Operator Algebras (math.OA)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics

description: We show that the $\ca$-envelope of the tensor algebra of an arbitrary $\ca$-correspondence $\X$ coincides with the Cuntz-Pimsner algebra $Ø_{\X}$, as defined by Katsura \cite{Ka}. This improves earlier results of Muhly and Solel and Fowler, Muhly and Raeburn, who came to the same conclusion under the additional hypothesis that $\X$ is strict and faithful.
description: 9 pages, final version, Journal of Functional Analysis, to appear
title: 01_1526
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: Laboratoire de Médiévistique Occidentale de Paris
subject: LaMOP

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/
Speech as Interactive Design Material (SIDM): How to design and evaluate task-tailored synthetic voices?
Creators: name: Dubiel, Mateusz
name: Aylett, Matthew
name: Schmitt, Anuschka
name: Ma, Zilin
name: Hsieh, Gary
name: Wambsganss, Thiemo
Publisher: name: arXiv
Year: 2024
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: The aim of this workshop is two-fold. First, it aims to establish a research community focused on design and evaluation of synthetic speech (TTS) interfaces that are tailored not only to goal oriented tasks (e.g., food ordering, online shopping) but also personal growth and resilience promoting applications (e.g., coaching, mindful reflection, and tutoring). Second, through discussion and collaborative efforts, to establish a set of practices and standards that will help to improve ecological validity of TTS evaluation. In particular, the workshop will explore the topics such as: interaction design of voice-based conversational interfaces; the interplay between prosodic aspects (e.g., pitch variance, loudness, jitter) of TTS and its impact on voice perception. This workshop will serve as a platform on which to build a community that is better equipped to tackle the dynamic field of interactive TTS interfaces, which remains understudied, yet increasingly pertinent to everyday lives of users.
description: Authors' preprint
Additional file 1 of Effectiveness of telerehabilitation intervention to improve pain and physical function in people with patellofemoral pain syndrome: study protocol for a randomized controlled trial
Creators: name: Amirabadi, Negar
name: Hessam, Masumeh
name: Monjezi, Saeideh
name: Molhemi, Farshad
name: Mehravar, Mohammad
name: Hosseinpour, Pardis
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Developmental Biology
subject: Science Policy
subject: Mental Health

description: Additional file 1. SPIRIT checklist.
NNLO corrections to massive lepton-pair production in longitudinally polarized proton-proton collisions
Creators: name: Ravindran, V.
name: Smith, J.
name: van Neerven, W. L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present the full next-to-next-to-leading order (NNLO) coefficient functions for the polarized cross section $dΔσ/dQ$ for the Drell-Yan process $p + p\to l^+l^- + 'X'$. Here $'X'$ denotes any inclusive hadronic state and $Q$ represents the invariant mass of the lepton pair. All QCD partonic subprocesses have been included provided the lepton pair is created by a virtual photon, which is a valid approximation for $Q<50$ GeV. Unlike the differential distribution w.r.t. transverse momentum the dominant subprocess for the integrated cross section is given by $q+\bar q \to γ^* + 'X'$ and its higher order corrections so that massive lepton pair production provides us with an excellent tool to measure the polarized anti-quark densities. Our calculations are carried out using the method of $n$-dimensional regularization by making a special choice for the $γ_5$ matrix. We give predictions for double longitudinal spin asymmetry measurements at the RHIC.
description: 45 pages, 22 figures. Due to a bug in our program the mass factorization plots in fig. 8-11 are changed. All parton density sets, in particular the set BB1 (J. Blumlein, H. Bottcher), lead to an improvement in the scale dependence while going from LO to NLO and then to NNLO
Various items relating to Robert Allan Yorston
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 items relate to the service of Robert Allan Yorston as a pilot in WWII. He was a student when war broke out and became a pilot in Coastal Command. He didn't take part in the Battle of Britain.He took his pilot training in South Africa before spending time in Cornwall and Iceland. He escorted convoys and undertook submarine patrols. His 269 Squadron got a submarine to surrender. He was awarded the Arctic Star medal.In 1995, he attended a reunion at Calderas Airfield in Iceland, although Icelanders had mixed feelings about the pilots during the war, as they were neutral.After the war, he returned to his studies and became an ENT surgeon. He retired in 1985 and died in 2016 at the age of 96.He left behind a wealth of material related to his war service, including log books, photo albums, medals, and heliographs.
Pions as Gluons in Higher Dimensions
Creators: name: Cheung, Clifford
name: Remmen, Grant N.
name: Shen, Chia-Hsien
name: Wen, Congkao
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We derive the nonlinear sigma model as a peculiar dimensional reduction of Yang-Mills theory. In this framework, pions are reformulated as higher-dimensional gluons arranged in a kinematic configuration that only probes cubic interactions. This procedure yields a purely cubic action for the nonlinear sigma model which exhibits a symmetry enforcing color-kinematics duality. Remarkably, the associated kinematic algebra originates directly from the Poincare algebra in higher dimensions. Applying the same construction to gravity yields a new quartic action for Born-Infeld theory and, applied once more, a cubic action for the special Galileon theory. Since the nonlinear sigma model and special Galileon are subtly encoded in the cubic sectors of Yang-Mills theory and gravity, respectively, their double copy relationship is automatic.
description: fixed typos and references in v2. Matched to JHEP version in v3
Roccella tinctoria
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Fungi
Ascomycota
Arthoniomycetes
Arthoniales
Roccellaceae
Roccella
Roccella tinctoria

description: Lichen roccella Linnaeus, Species Plantarum 2: 1154. 1753.
"Habitat in insulis Archipelagi, Canariis, ad rupes marinas." RCN: 8244.
 Lectotype (Howe in Bull. Torrey Bot. Club 39: 201. 1912; Jørgensen & al. in Bot. J. Linn. Soc. 115: 350, f. 55. 1994): Herb. Linn. No. 1273.263, lower specimen (LINN).
 Current name: Roccella tinctoria DC. (Roccellaceae).
 Note: Jørgensen & al. (in Bot. J. Linn. Soc. 115: 350, 380, f. 55. 1994) restricted Howe’s original type choice to one of the specimens on the sheet.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 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 630, DOI: 10.5281/zenodo.291971
Star-forming QSO host galaxies
Creators: name: Barthel, P. D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent finding of substantial masses of cold molecular gas as well as young stellar populations in the host galaxies of quasars is at odds with results of Hubble Space Telescope imaging studies, since the latter appear to yield mature, quiescent early type hosts. It is demonstrated here that the characterization as `quiescent' is incorrect. Radio and far-infrared properties of both the HST sample and a larger comparison sample of uv-excess selected radio-quiet QSOs are consistent with substantial recent star-formation activity.
description: Accepted for publication by Astronomy & Astrophysics
53 | Supplemento | 2019
Creators: name: Cortesi, Luca
name: Cugnata, Cristina
name: De Capitani, Lucio
name: Frare, Giulia
name: Girotto, Alice
name: Vianello, Serena
Publisher: name: Università Ca’ Foscari Venezia, Italia
Year: 2019

description:

Progetti per l’Umanità. Rivoluzioni, Utopie e Ingegneria Sociale (Projects for Humankind. Revolutions, Utopias and Social Engineering) explores a variety of plans and attempts to transform human beings into something different and better. In particular, it engages with utopian thinking and its ineludible counterpart, dystopia; with moments of political, cultural or philosophical revolution aimed at triggering profound shifts in human life; and with different projects of social engineering to be accomplished through a variety of means such as education, propaganda or alterations to the human body or mind. The case studies included in this volume range from the 18th century to the present day, and involve disciplines such as literary and film studies, philosophy, political science and cultural history. In particular, the volume features essays on the following topics: mythology in German Romanticism; Martin Heidegger’s eschatology; Francesco Saverio Salfi’s essay on the 1783 earthquake in Calabria; the scapigliati writers Carlo Dossi and Giovanni Faldella; the utopian production of positivist anthropologist Paolo Mantegazza; the Proletkul’t movement; early Soviet children’s magazines; the political implications of Russian linguaculturology (lingvokul’turologija); Lafayette Ronald Hubbard’s Dianetics; Zulu intellectual and writer Herbert Dhlomo’s speculative fiction; “self-management” (autogestione) and the Italian Socialist Party in the 1970s; the current debate on surrogate motherhood; and Terry Gilliam’s dystopian film trilogy. Through these multiple perspectives, the volume argues that human projectuality is an anthropological constant throughout history that is both necessary for human existence and simultaneously fraught with dangers; and that it is therefore a crucial category to analyse reality and fiction alike.

description: Annali di Ca’ Foscari. Serie occidentale
On The Metal-poor non-Sagittarius Globular Cluster NGC 5053: Orbit, Mg, Al, and Si
Creators: name: Tang, Baitian
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Metal-poor globular clusters (GCs) show intriguing Al-Mg and Si-Al correlations, which are important clues to decipher the multiple population phenomenon. NGC 5053 is one of the most metal-poor GCs, and has been suggested to be associated with the Sagittarius dwarf galaxy (Sgr), due to its similar location and radial velocity with one of the Sgr arms. In this work, we simulate the orbit of NGC 5053, and argue against the connection between Sgr and NGC 5053. Meanwhile, Mg, Al, and Si spectral lines, which are difficult to detect in the optical spectra, have been detected in the near-infrared APOGEE spectra. We use three different sets of stellar parameters and codes to derive the Mg, Al, and Si abundances, and we always see a large Al variation, and a substantial Si enhancement. Comparing with other metal-poor GCs, we suggest metallicity may not be the only parameter that controls the multiple populations.
description: IAU 334 symposium proceeding, 2 pages
Surveying capsid assembly pathways through simulation-based data fitting.
Creators: name: Xie, Lu
name: Smith, Gregory R.
name: Feng, Xian
name: Schwartz, Russell
Publisher: name: Carnegie Mellon University
Year: 2012
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Virus capsid assembly has attracted considerable interest from the biophysical modeling community as a model system for complicated self-assembly processes. Simulation methods have proven valuable for characterizing the space of possible kinetics and mechanisms of capsid assembly, but they have so far been able to say little about the assembly kinetics or pathways of any specific virus. It is not possible to directly measure the detailed interaction rates needed to parameterize a model, and there is only a limited amount of experimental evidence available to constrain possible pathways, with almost all of it gathered from in vitro studies of purified coat proteins. In prior work, we developed methods to address this problem by using simulation-based data-fitting to learn rate parameters consistent with both structure-based rule sets and experimental light-scattering data on bulk assembly progress in vitro. We have since improved these methods and extended them to fit simulation parameters to one or more experimental light-scattering curves. Here, we apply the improved data-fitting approach to three capsid systems-human papillomavirus (HPV), hepatitis B virus (HBV), and cowpea chlorotic mottle virus (CCMV)-to assess both the range of pathway types the methods can learn and the diversity of assembly strategies in use between these viruses. The resulting fits suggest three different in vitro assembly mechanisms for the three systems, with HPV capsids fitting a model of assembly via a nonnucleation-limited pathway of accumulation of individual capsomers while HBV and CCMV capsids fit similar but subtly different models of nucleation-limited assembly through ensembles of pathways involving trimer-of-dimer intermediates. The results demonstrate the ability of such data fitting to learn very different pathway types and show some of the versatility of pathways that may exist across real viruses.
S wave meson spectra from the light cone harmonic oscillator model with a consistent hyperfine interaction
Creators: name: Zhou, Shan-Gui
name: Pauli, Hans-Christian
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We use a light cone harmonic oscillator model to study S wave meson spectra, namely the pseudoscalar and vector mesons. The model Hamiltonian is a mass squared operator consisting of a central potential (a harmonic oscillator potential) from which a hyperfine interaction is derived. The hyperfine interaction is responsible for the splitting in the pseudoscalar-vector spectra. With 4 parameters for the masses of up/down, strange, charm and bottom quarks, 2 for the harmonic oscillator potential and 1 for the hyperfine interaction, the model presents a reasonably good agreement with the data.
description: 4 pages, no figures, RevTeX4; v2: typo in the title removed
ALMA Observations of Circumnuclear Disks in Early Type Galaxies: 12CO(2-1) and Continuum Properties
Creators: name: Boizelle, Benjamin D.
name: Barth, Aaron J.
name: Darling, Jeremy
name: Baker, Andrew J.
name: Buote, David A.
name: Ho, Luis C.
name: Walsh, Jonelle
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present results from an Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 2 program to map CO(2-1) emission in nearby early-type galaxies (ETGs) that host circumnuclear gas disks. We obtained $\sim0.3''-$resolution Band 6 observations of seven ETGs selected on the basis of dust disks in Hubble Space Telescope images. We detect CO emission in five at high signal-to-noise ratio with the remaining two only faintly detected. All CO emission is coincident with the dust and is in dynamically cold rotation. Four ETGs show evidence of rapid central rotation; these are prime candidates for higher-resolution ALMA observations to measure the black hole masses. In this paper we focus on the molecular gas and continuum properties. Total gas masses and H$_2$ column densities for our five CO-bright galaxies are on average $\sim10^8$ $M_\odot$ and $\sim10^{22.5}$ cm$^{-2}$ over the $\sim$kpc-scale disks, and analysis suggests that these disks are stabilized against gravitational fragmentation. The continuum emission of all seven galaxies is dominated by a central, unresolved source, and in five we also detect a spatially extended component. The $\sim$230 GHz nuclear continua are modeled as power laws ranging from $S_ν\sim ν^{-0.4}$ to $ν^{1.6}$ within the observed frequency band. The extended continuum profiles of the two radio-bright (and CO-faint) galaxies are roughly aligned with their radio jet and suggests resolved synchrotron jets. The extended continua of the CO-bright disks are coincident with optically thick dust absorption and have spectral slopes that are consistent with thermal dust emission.
description: 20 pages, 10 figures; accepted for publication in ApJ
Additional file 1 of Impact of an oral care subsidization reform on intersectional inequities in self-rated oral health in Sweden
Creators: name: Anticona, Cynthia
name: Suominen, Anna Liisa
name: Holgerson, Pernilla Lif
name: Gustafsson, Per E
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Supplementary Material 1
Additional file 1 of Bidirectional association between knee osteoarthritis and depressive symptoms: evidence from a nationwide population-based cohort
Creators: name: Lu, Han
name: Wang, Limin
name: Zhou, Weijiao
name: Jin, Shida
name: Chen, Hongbo
name: Su, Yi
name: Li, Nan
name: Shang, Shaomei
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: Additional file 1. Supplementary materials. Table S1-S6.
Subthreshold glutamate release from mitral cell dendrites.
Creators: name: Castro, Jason B.
name: Urban, Nathan
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: The dendrites of a number of neuron types function as presynaptic structures, releasing transmitter after action potentials and dendritic spikes. In this regard, dendrites can function like axons, producing discrete outputs after suprathreshold electrical events. However, as the major site of synaptic inputs, dendrites experience ongoing subthreshold fluctuations in membrane potential, raising the question of whether these subthreshold changes can cause changes in transmitter release. Here, we show that mitral cells of the accessory olfactory bulb release glutamate from their dendrites in response to both subthreshold and suprathreshold stimuli. Whereas subthreshold output was typically low under control conditions, it could be enhanced several fold by pharmacological or endogenous activation of group I metabotropic glutamate receptors. These results indicate that presynaptic dendrites can support two distinct forms of output, and can dynamically regulate how electrical activity is coupled to transmitter release.
A conditionally integrable bi-confluent Heun potential involving inverse square root and centrifugal barrier terms
Creators: name: Ishkhanyan, T. A.
name: Krainov, V. P.
name: Ishkhanyan, A. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a conditionally integrable potential, belonging to the bi-confluent Heun class, for which the Schrödinger equation is solved in terms of the confluent hypergeometric functions. The potential involves an attractive inverse square root term with arbitrary strength and a repulsive centrifugal barrier core with the strength fixed to a constant. This is a potential well defined on the half-axis. Each of the fundamental solutions composing the general solution of the Schrödinger equation is written as an irreducible linear combination, with non-constant coefficients, of two confluent hypergeometric functions. We present the explicit solution in terms of the non-integer order Hermite functions of scaled and shifted argument and discuss the bound states supported by the potential. We derive the exact equation for the energy spectrum and approximate that by a highly accurate transcendental equation involving trigonometric functions. Finally, we construct an accurate approximation for the bound-state energy levels.
The role of microquasars in astroparticle physics
Creators: name: Chaty, Sylvain
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena and astroparticle physics. After reminding the analogy with quasars, I focus on one of the best microquasar representatives, probably the archetype, namely GRS 1915+105, and present accretion and ejection phenomena, showing that only a multi-wavelength approach allows a better understanding of phenomena occurring in these sources. Thereafter, I review jets at different scales: compact jets, large-scale jets, and the interactions between ejection and the surrounding medium. I finish this review by showing that microquasars are good candidates to be emitters of astroparticles: very high energy photons, cosmic rays and neutrinos.
description: Invited review at Frontier Objects in Astrophysics and Particle Physics, Vulcano (Italy) 22nd - 27th May, 2006, 12 pages, 4 figures
title: 03_0907
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/
Additional file 7 of Quantitative redox proteomics revealed molecular mechanisms of salt tolerance in the roots of sugar beet monomeric addition line M14
Creators: name: Liu, He
name: Du, Xiaoxue
name: Zhang, Jialin
name: Li, Jinna
name: Chen, Sixue
name: Duanmu, Huizi
name: Li, Haiying
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 7: Table S6. The transcriptional level, redox protein level of 14 differential redox proteins.
The Spectral Energy Distribution of Dust Emission in the Edge-on Spiral Galaxy NGC 4631 as seen with Spitzer and JCMT
Creators: name: Bendo, George J.
name: Dale, Daniel A.
name: Draine, Bruce T.
name: Engelbracht, Charles W.
name: Kennicutt,, Robert C.
name: Calzetti, Daniela
name: Gordon, Karl D.
name: Helou, George
name: Hollenbach, David
name: Li, Aigen
name: Murphy, Eric J.
name: Prescott, Moire K. M.
name: Smith, John-David T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We explore the nature of variations in dust emission within an individual galaxy using 3.6 - 160 micron Spitzer Space Telescope observations and 450 and 850 micron James Clerk Maxwell Telescope observations of the edge-on Sd spiral galaxy NGC 4631 with the goals of understanding the relation between polycyclic aromatic hydrocarbons (PAH) and dust emission, studying the variations in the colors of the dust emission, and searching for possible excess submillimeter emission compared to what is anticipated based on dust models applied to the mid- and far-infrared data. PAH emission at 8 micron is found to correlate best with hot dust emission at 24 micron on kiloparsec scales, although the relation breaks down on scales equal to hundreds of parsecs, possibly because of differences in the mean free paths between the photons that excite the PAHs and heat the dust and possibly because the PAHs are destroyed by the hard radiation fields in the centers of some star formation regions. The ratio of 8 micron PAH emission to 160 micron cool dust emission appears to be a function of radius. The 70/160 and 160/450 micron flux density ratios are remarkably constant even though the surface brightness varies by a factor of 25 in each wave band, which suggests that the emission is from dust heated by a nearly-uniform radiation field. Globally, we find an excess of 850 micron emission relative to what would be predicted by dust models. The 850 micron excess is highest in regions with low 160 micron surface brightness, although the strength and statistical significance of this result depends on the model fit to the data. We rule out variable emissivity functions or ~4 K dust as the possible origins of this 850 micron emission, but we do discuss the other possible mechanisms that could produce the emission.
description: Accepted to the Astrophysical Journal
การวิเคราะห์เป้าหมายและวิเคราะห์งานสอนของเนื้อหาการเขียนสื่อความเพื่อพัฒนาทักษะการเขียนภาษาไทยสำหรับนักศึกษาชาวต่างประเทศ
Creators: name: สุภา พูนผล
name: เกียรติสุดา บุญส่ง
Publisher: name: วารสารมหาวิทยาลัยพายัพ
Year: 2019
Subjects: การวิเคราะห์งานสอน
การเขียนสื่อความ
การพัฒนาทักษะการเขียนภาษาไทย
นักศึกษาชาวต่างประเทศ

description: วารสารมหาวิทยาลัยพายัพ, 29, 2, 147
An Overview of the Anomaly-Induced Inflation
Creators: name: Shapiro, Ilya L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The anomaly-induced inflation (modified Starobinsky model) is based on the application of the effective quantum field theory approach to the Early Universe. We present a brief general review of this model with a special attention to the existing difficulties and unsolved problems.
description: Talk presented at IRGA2003 (Renormalization Group and Anomalies in Gravitation and Cosmology, Ouro Preto, Brazil, 16-23 March, 2003)
title: ADCO, Cart. 186 (11 H 71), f. 0374r
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0374r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-
project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Explicit triangular decoupling of the separated vector wave equation on Schwarzschild into scalar Regge-Wheeler equations
Creators: name: Khavkine, Igor
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We consider the vector wave equation on the Schwarzschild spacetime, which can be considered as coming from the harmonic (or Lorenz) gauge fixed Maxwell equations. After a separation of variables, the radial mode equations form a complicated system of coupled linear ODEs. We outline a precise abstract strategy to decouple this system into triangular form, where the diagonal blocks consist of spin-$s$ scalar Regge-Wheeler equations, with $s=0$ or $1$. This strategy is then implemented to give an explicit transformation of the radial mode equations (with nonzero frequency and angular momentum) into this triangular form. Our decoupling goes a step further than previous results in the literature by making the triangular form explicit and reducing it as much as possible. Also, with the help of our abstractly formulated decoupling strategy, we have significantly streamlined both the presentation of the final results and the intermediate calculations. Finally, we note that the vector wave equation is a simple model for more complicated equations, like harmonic (or de Donder) gauge fixed linearized gravity, and backgrounds, like Kerr, where we expect the same abstract decoupling strategy to work as well.
description: v2: improved notation, fixed some inconsistent formulas; close to published version, with minor further corrections. v1: 20 pages, no figures; contribution to the proceedings of the workshop "Non-regular spacetime geometry" held in Florence, Italy, 20-22 Jun 2017
Systematic screening of different polyglycerin‐based dienophile macromonomers for efficient nanogel formation through IEDDA inverse nanoprecipitation
Creators: name: Oehrl, Alexander
name: Haag, Rainer
name: Schötz, Sebastian
Publisher: name: Freie Universität Berlin
Year: 2019
Subjects: subject: inverse electron demand Diels Alder
subject: nanogels
subject: nanoprecipitation
subject: protein encapsulation
subject: 500 Naturwissenschaften und Mathematik::540 Chemie::547 Organische Chemie

description: Alternatives for strain‐promoted azide–alkyne cycloaddition (SPAAC) chemistries are needed because of the employment of expensive and not easily scalable precursors such as bicyclo[6.1.0]non‐4‐yne (BCN). Inverse electron demand Diels Alder (iEDDA)‐based click chemistries, using dienophiles and tetrazines, offer a more bioorthogonal and faster toolbox, especially in the biomedical field. Here, the straightforward synthesis of dendritic polyglycerin dienophiles (dPG‐dienophiles) and dPG‐methyl‐tetrazine (dPG‐metTet) as macromonomers for a fast, stable, and scalable nanogel formation by inverse nanoprecipitation is reported. Nanogel size–influencing parameters are screened such as macromonomer concentration and water‐to‐acetone ratio are screened. dPG‐norbonene and dPG‐cyclopropene show fast and stable nanogel formation in the size range of 40–200 nm and are thus used for the coprecipitation of the model protein myoglobin. High encapsulation efficiencies of more than 70% at a 5 wt% feed ratio are obtained in both cases, showing the suitability of the mild gelation chemistry for the encapsulation of small proteins.
Subdivision of large introns in Drosophila by recursive splicing at nonexonic elements.
Creators: name: Burnette, James M.
name: Miyamoto-Sato, Etsuko
name: Schaub, Marc A.
name: Conklin, Jamie
name: Antonio-Javier Lopez
Publisher: name: Carnegie Mellon University
Year: 2005
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Many genes with important roles in development and disease contain exceptionally long introns, but special mechanisms for their expression have not been investigated. We present bioinformatic, phylogenetic, and experimental evidence in Drosophila for a mechanism that subdivides many large introns by recursive splicing at nonexonic elements and alternative exons. Recursive splice sites predicted with highly stringent criteria are found at much higher frequency than expected in the sense strands of introns >20 kb, but they are found only at the expected frequency on the antisense strands, and they are underrepresented within intronspseudoobscura, despite extensive divergence of other sequences within the same introns. These patterns of enrichment and conservation indicate that recursive splice sites are advantageous in the context of long introns. Experimental analyses of in vivo processing intermediates and lariat products from four large introns in the unrelated genes kuzbanian, outspread, and Ultrabithorax confirmed that these introns are removed by a series of recursive splicing steps using the predicted nonexonic sites. Mutation of nonexonic site RP3 within Ultrabithorax also confirmed that recursive splicing is the predominant processing pathway even with a shortened version of the intron. We discuss currently known and potential roles for recursive splicing.