cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Determination of the transverse velocity of Q2237+0305
Creators: name: Wyithe, J. S. B.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The largest systematic uncertainty present in the analysis of gravitationally microlensed quasar light curves is that of the galactic transverse velocity. We describe a method for determining the transverse velocity as well as its application to published monitoring data of Q2237+0305 (Irwin et al. 1989; Corrigan et al. 1991; Ostensen et al 1995). We find that while this data displays strong evidence for microlensing, it limits the transverse velocity to be < 500 km/sec (for microlens masses of 0.5 solar masses). In addition, by combining these results with a new method for modelling the microlensing contribution of stellar proper motions, we find that the masses of microlenses in Q2237+0305 are consistent with those of low mass stars.
description: 4 pages, 2 figures. To appear in "Gravitational Lensing: Recent Progress and Future Goals", ASP conference series, eds Brainerd & Kochanek
Vanilla yanesha Damian-Parizaca
Creators: name: Damián-Parizaca, Alexander
name: Karremans, Adam P.
name: Mitidieri-Rivera-Rivera, Nicole
name: Cameron, Kenneth M.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Vanilla
Vanilla yanesha

description: 29.Vanilla yaneshaDamián-Parizaca (Damián-Parizaca 2019: 5)
Type.
PERU – Pasco • Oxapampa; Palcazu, San Francisco de Pichanaz; 550 m a. s. l.; bosque secundario; 28 Feb. 2006; R. Rojas, J. Mateo & C. Rojas 3947; holotype: USM! [USM 240875]; isotypes: HOXA! [HOXA 126525], MO! [MO 6049740].
description: Published as part of Damián-Parizaca, Alexander, Karremans, Adam P., Mitidieri-Rivera-Rivera, Nicole & Cameron, Kenneth M., 2025, Towards a monograph of membranaceous Vanillas: a nomenclatural revision of Vanilla subgen. Vanilla (Vanilloideae, Orchidaceae), pp. 111-121 in Plant Ecology and Evolution 158 (1) on pages 111-121, DOI: 10.5091/plecevo.140667
Electron-ion model of ball and bead lightning
Creators: name: Fedosin, Sergey G.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: Based on the electron-ion model, parameters of ball and bead lightning are calculated. The model allows us to estimate maximum size of ball lightning, its energy content, electric charge and magnetic field, to determine equilibrium conditions between positively charged ions located inside and outer shell containing rapidly moving electrons. An explanation is given to the fact that shells are observed inside ball lightning that differ from each other in color of glow. The model describes structure of not only ball lightning, but also bead lightning. The long-term stability of bead lightning is associated with the balance of neighboring beads under action of magnetic force of their attraction and electric force of repulsion, which exceed in magnitude the force of wind pressure.
description: 34 pages
MOESM6 of Reduced-representation sequencing identifies small effective population sizes of Anopheles gambiae in the north-western Lake Victoria basin, Uganda
Creators: name: Wiltshire, Rachel
name: Bergey, Christina
name: Kayondo, Jonathan
name: Birungi, Josephine
name: Mukwaya, Louis
name: Emrich, Scott
name: Besansky, Nora
name: Collins, Frank
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 6: Figure S2. ADMIXTURE bar plot of chromosome 2L SNPs (K = 2) showing probable ancestry fractions of the six An. gambiae populations (N = 79) based on the 2La inversion.
Thermal Instability and Photoionized X-ray Reflection in Accretion Disks
Creators: name: Nayakshin, Sergei
name: Kazanas, Demosthenes
name: Kallman, Timothy R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the X-ray illumination of an accretion disk. We relax the simplifying assumption of constant gas density used in most previous studies; instead we determine the density from hydrostatic balance. It is found that the thermal ionization instability prevents the illuminated gas from attaining temperatures at which the gas is unstable. In particular, the uppermost layers of the X-ray illuminated gas are found to be almost completely ionized and at the local Compton temperature ($\sim 10^7 - 10^8$ K); at larger depths, the gas temperature drops abruptly to form a thin layer with $T\sim 10^6$ K, while at yet larger depths it decreases sharply to the disk effective temperature. We find that most of the Fe K$α$ line emission and absorption edge are produced in the coolest, deepest layers, while the Fe atoms in the hottest, uppermost layers are generally almost fully ionized, hence making a negligible contribution to reprocessing features in $\sim 6.4-10$ keV energy range. We provide a summary of how X-ray reprocessing features depend on parameters of the problem. The results of our self-consistent calculations are both quantitatively and qualitatively different from those obtained using the constant density assumption. Therefore, we conclude that X-ray reflection calculations should always utilize hydrostatic balance in order to provide a reliable theoretical interpretation of observed X-ray spectra of AGN and GBHCs.
description: Submitted to ApJ; 16 pages plus 13 figures
title: Joseph und Helene am 1. Mai?
Creators: name: Neumeier, Daniel
Publisher: name: ZZF - Leibniz-Zentrum für Zeithistorische Forschung: Visual History
Year: 2024

description: Auf dem vorliegenden Bild posiert Joseph vor einem Lastwagen. Helene schaut zusammen mit einem Kind aus der Fahrerkabine in die Kamera. Auf der Ladefläche stehen weitere Kinder sowie eine abgeschnittene größere Person. Die Abgebildeten tragen weiße Hemden und einige der Kinder auch weiße Hüte – sie wirken aufgeregt. Mindestens zwei der Kinder halten kleine einfarbige Fahnen in ihren Händen.
Lettre de Frère Gabriel d'Aix à Jean-François Séguier, 1767-01-16
Creators: name: Aix, Frère Gabriel d'
name: Frère Gabriel D'Aix
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Botanique

description: [transcription] De la Tour d'Aigues 16e janvier 1767

[Gabriel]

Monsieur,

Il est très juste qu'après un si long silence envers vous, je vienne le rompre dans cette nouvelle année et ce ne sera que pour vous assurer que les voeux que je fais pour vous, Monsieur, à cette occasion, sont des plus ardents et des plus sincères. Daigne le ciel les exaucer et vous conserver longues années en santé la plus parfaite. J'aurais l'honneur maintenant de vous parler un peu de botanique. Premièrement, j'ai envoyé le catalogue des graines que j'ai à Monsierur Gouan, le priant de vous le faire parvenir pour que vous marquiez les graines qu'ils vous feront plaisir pour que je vous les envoye tout de suite par la voie de Monsieur Girard.

Le Père dom Jean-François Maratti, professeur de botanique à Rome, me fait l'honneur de m'écrire quelques fois, de m'envoyer des graines et de me marquer les découvertes qu'il fait en plantes. Il a découvert dans la marche d'Ancône un rosier en arbre dont le pied à un pan et demi de diamètre. La fleur est d'un jaune pâle. Tout l'arbre est sans épines. Un sorbus qu'il appelle sorbus umbellatus foliis simplicibus avatio acuminatis, in ambitu serratis, unipleuris, pleura ad latus ramosa, ramis simplicibus, et dichotomis; est arbor procera per dichotomiam divisa. Un Iumiperus parvus foliis superioribussabinam referentibus inferioribus ex ovato-acuminatis. Un faeniculum foliis caulinis compositis lobis rachi adversa tri et pentanatis, pariter adversis oblongo-ovatis, acumina terminatis, integerrimis. Un [fol. 108 v] allium parvum hyemale acaulos, floribus albis, Linea viridi notatis. Un arbrisseau qu'il appelle vetula et plusieurs autres, ainsi vous voyez que c'est un zélé professeur de botanique quoi qu'ilne donne guère au public.

Monsieur le baron de La Tour d'Aigues me fait la grâce de me tenir son château pour y achever un herbier auquel je travaille et je compte achever bientôt. Si vous aviez des graines sà pouvoir me faire la grâce de me communiquer qui ne fussent point sur mon catalogue, vous m'obligeriez beaucoup. Je finis en osant vous prier de faire agréer mes soumissions à Monsieur le chanoine votre frère et à Mademoiselle votre soeur. J'ai l'honneur d'être avec respect,

Monsieur,

Votre très humble et très obéissant serviteur

Fr. Gabriel religieux capucin.

[fol. 109 r] [16e janvier 1767, Gabriel]
description: [note autre main] [16e janvier 1767, Gabriel]
description: [personnes citées] Antoine Gouan, Barthélemy Girard, Giovanni Francesco Maratti, Jean Baptiste Jérôme de Bruny, baron de La Tour d'Aigues, Joseph Maximilien Séguier, Marianne Séguier
description: Source: [lieu de Conservation] Nîmes, Bibliothèque Carré d'Art [cote]ms. 94_9, fol. 108-109
description: Source: ark:/12148/btv1b10015079m
Polarization and Anisotropy of the Microwave Sky
Creators: name: Coulson, David
name: Crittenden, Robert G.
name: Turok, Neil
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the polarization-polarization and polarization-temperature correlations in standard adiabatic scenarios for structure formation. Temperature anisotropies due to gravitational potential wells and oscillations in the photon-baryon-electron fluid on the surface of last scattering are each associated with a correlated polarization pattern. While the `correlated part' of the polarization has an r.m.s. of only a third of the total signal, it may still be measurable by mapping a large area on the sky. We calculate the expected signal to noise ratio for various measures of the polarization in a hypothetical mapping experiment such as those now being planned.
description: 12 pages of uuencoded compressed postscript (replacing previous uncompressed version), figures included. PUPT-94-1473
Corallina penicillus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Sabellidae
Corallina
Corallina penicillus

description: Corallina penicillus [spec. nov.]
C. culmo simplici, ramis fasciculatis fastigiatis dichotomis flexilibus inarticulatis.
Habitat in Asia.
Stirps crassitie pennae, longitudine digiti, cortice fere tectus, e cujus apice, penicilli instar, fasciculus ramorum filiformium.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 807, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Caltech Faint Field Galaxy Redshift Survey IX: Source detection and photometry in the Hubble Deep Field Region
Creators: name: Hogg, David W.
name: Pahre, Michael A.
name: Adelberger, Kurt L.
name: Blandford, Roger
name: Cohen, Judith G.
name: Gautier, T. N.
name: Jarrett, Thomas
name: Neugebauer, Gerry
name: Steidel, Charles C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Detection and photometry of sources in the U_n, G, R, and K_s bands in a 9x9 arcmin^2 region of the sky, centered on the Hubble Deep Field, are described. The data permit construction of complete photometric catalogs to roughly U_n=25, G=26, R=25.5 and K_s=20 mag, and significant photometric measurements somewhat fainter. The galaxy number density is 1.3x10^5 deg^{-2} to R=25.0 mag. Galaxy number counts have slopes dlog N/dm=0.42, 0.33, 0.27 and 0.31 in the U_n, G, R and K_s bands, consistent with previous studies and the trend that fainter galaxies are, on average, bluer. Galaxy catalogs selected in the R and K_s bands are presented, containing 3607 and 488 sources, in field areas of 74.8 and 59.4 arcmin^2, to R=25.5 and and K_s=20 mag.
description: Accepted for publication in ApJS; some tables and slightly nicer figures available at http://www.sns.ias.edu/~hogg/deep/
On the Spontaneous CP Breaking at Finite Temperature in a Nonminimal Supersymmetric Standard Model
Creators: name: Comelli, D.
name: Pietroni, M.
name: Riotto, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the spontaneous CP breaking at finite temperature in the Higgs sector in the Minimal Supersymmetric Standard Model with a gauge singlet. We consider the contribution of the standard model particles and that of stops, charginos, neutralinos, charged and neutral Higgs boson to the one-loop effective potential. Plasma effects for all bosons are also included. Assuming CP conservation at zero temperature, so that experimental constraints coming from, {\it e.g.}, the electric dipole moment of the neutron are avoided, and the electroweak phase transition to be of the first order and proceeding via bubble nucleation, we show that spontaneous CP breaking cannot occur inside the bubble mainly due to large effects coming from the Higgs sector. However, spontaneous CP breaking can be present in the region of interest for the generation of the baryon asymmetry, namely inside the bubble wall. The important presence of very tiny explicit CP violating phases is also commented.
description: 28 pages, 4 figures available upon request, DFPD 94/TH/38 and SISSA 94/81-A preprints
Sensitive Radio Observations of High Redshift Dusty QSOs
Creators: name: Yun, M. S.
name: Carilli, C. L.
name: Kawabe, R.
name: Tutui, Y.
name: Kohno, K.
name: Ohta, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present sensitive radio continuum imaging at 1.4 GHz and 4.9 GHz of seven high redshift QSOs selected for having a 240 GHz continuum detection, which is thought to be thermal dust emission. We detect radio continuum emission from four of the sources: BRI 0952-0115, BR 1202-0725, LBQS 1230+1627B, and BRI 1335-0417. The radio source in BR 1202-0725 is resolved into two components, coincident with the double mm and CO sources. We compare the results at 1.4 GHz and 240 GHz to empirical and semi-analytic spectral models based on star forming galaxies at low redshift. The radio-to-submm spectral energy distribution for BR 1202-0725, LBQS 1230+1627B, and BRI 1335-0417 are consistent with that expected for a massive starburst galaxy, with implied massive star formation rates of order 1000 solar masses per year (without correcting for possible amplification by gravitational lensing). The radio-to-submm spectral energy distribution for BRI 0952-0115 suggests a low-luminosity radio jet source driven by the AGN.
description: 12 pages, Latex emulateapj format, including 1 table and 3 figures. The Astrophysical Journal, to appear in the January 2000 issue
Statistical Constraints on the Inflation Effective Potential from the COBE DMR Results
Creators: name: Kurki-Suonio, Hannu
name: Mathews, Grant J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We explore constraints on various forms for the effective potential during inflation based upon a statistical comparison between inflation-generated fluctuations in the cosmic microwave background temperature and the COBE DMR results. Fits to the first year 53 A + B x 90 A + B cross correlation function using an effective potential of the form V(phi) = lambda*phi^x/x!, yield upper limits of x le 107 and x le 397 at the 1 sigma and 2 sigma confidence levels, while the same analysis produces a power law of index of n = 1.10 ^{+0.47}_{-0.64} which would imply an underestimate of x le 63 from the simple analytic relation between x and n . We also quantify new limits on the parameters for polynomial effective potentials. This work highlights the importance of a careful statistical treatment when seeking constraints on the inflation-generating effective potential.
description: 4 pages, uuencoded compressed ps file, accepted by Physical Review D, HU-TFT-94-16
MOESM5 of Reduced-representation sequencing identifies small effective population sizes of Anopheles gambiae in the north-western Lake Victoria basin, Uganda
Creators: name: Wiltshire, Rachel
name: Bergey, Christina
name: Kayondo, Jonathan
name: Birungi, Josephine
name: Mukwaya, Louis
name: Emrich, Scott
name: Besansky, Nora
name: Collins, Frank
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 5: Figure S1. (aâ d) PCA plots of An. gambiae chromosomes not shown in the main text.
Additional file 2 of m6A demethylase FTO promotes tumor progression via regulation of lipid metabolism in esophageal cancer
Creators: name: Duan, Xiaoran
name: Yang, Li
name: Wang, Liuya
name: Liu, Qinghua
name: Zhang, Kai
name: Liu, Shasha
name: Liu, Chaojun
name: Gao, Qun
name: Li, Lifeng
name: Qin, Guohui
name: Zhang, Yi
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 2: Figure S1. Esophageal cancer stem-like cells and survival analysis. A Representative images of the cell spheres in the ECCs; B qPCR analysis of the cell stemness markers and cell renewal factors after sphering of ECCs; C Flow cytometry detected the cell stemness markers CD90, CD133, and CD271, D the corresponding statistical results are presented; E Kaplan-Meier survival curves were used to analyze the effects of age, sex, pathological grade, tumor stage, and lymph node metastasis on the overall patient survival.
Deep 10 and 18 micron Imaging of the HR 4796A Circumstellar Disk: Transient Dust Particles & Tentative Evidence for a Brightness Asymmetry
Creators: name: Telesco, C. M.
name: Fisher, R. S.
name: Pina, R. K.
name: Knacke, R. F.
name: Dermott, S. F.
name: Wyatt, M. C.
name: Grogan, K.
name: Holmes, E. K.
name: Ghez, A. M.
name: Prato, L.
name: Hartmann, L. W.
name: Jayawardhana, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new 10.8 and 18.2 micron images of HR 4796A, a young A0V star that was recently discovered to have a spectacular, nearly edge-on, circumstellar disk prominent at ~20 microns (Jayawardhana et al. 1998; Koerner et al. 1998). These new images, obtained with OSCIR at Keck II, show that the disk's size at 10 microns is comparable to its size at 18 microns. Therefore, the 18 micron-emitting dust may also emit some, or all, of the 10 micron radiation. Using these multi-wavelength images, we determine a "characteristic" diameter of 2-3 microns for the mid-infrared-emitting dust particles if they are spherical and composed of astronomical silicates. Particles this small are expected to be blown out of the system by radiation pressure in a few hundred years, and therefore these particles are unlikely to be primordial. Dynamical modeling of the disk (Wyatt et al. 2000) indicates that the disk surface density is relatively sharply peaked near 70 AU, which agrees with the mean annular radius deduced by Schneider et al. (1999) from their NICMOS images. We present evidence (~1.8 sigma significance) for a brightness asymmetry that may result from the presence of the hole and the gravitational perturbation of the disk particle orbits by the low-mass stellar companion or a planet. This "pericenter glow," which must still be confirmed, results from a very small (a few AU) shift of the disk's center of symmetry relative to the central star HR 4796A; one side of the inner boundary of the annulus is shifted towards HR 4796A, thereby becoming warmer and more infrared-emitting. The possible detection of pericenter glow implies that the detection of even complex dynamical effects of planets on disks is within reach.
description: 18 pages. 9 GIF images. Total size ~800 kB. High resolution images available upon request. Accepted for publication in the Astrophysical Journal (scheduled for January 10, 2000)
On Spontaneous Baryogenesis and Transport Phenomena
Creators: name: Comelli, D.
name: Pietroni, M.
name: Riotto, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The spontaneous baryogenesis mechanism by Cohen, Kaplan and Nelson is reconsidered taking into account the transport of particles inside the electroweak bubble walls. Using linear response theory, we calculate the modifications on the thermal averages of the charges of the system due to the presence of a space time dependent `charge potential' for a quantum number not orthogonal to baryon number. The local equilibrium configuration is discussed, showing that, as a consequence of non zero densities for conserved charges, the $B+L$ density is driven to non zero values by sphaleronic processes. Solving a rate equation for the baryon number generation, we obtain an expression for the final baryon asymmetry of the Universe containing the relevant parameters of the bubble wall, {\it i.e.} its velocity, its width, and the width of the region in which sphalerons are active. Compared to previous estimates in which transport effects were not taken into account, we find an enhancement of nearly three orders of magnitude in the baryon asymmetry. Finally, the role of QCD sphalerons in cooperation with transport effects is analyzed, showing that the net result depends crucially on the particle species which enter into the charge potential.
description: 23 pages, 5 LaTeX figures, to be processed with feynman.tex, DFPD 94/TH/39
Keck Imaging of Binary L Dwarfs
Creators: name: Koerner, D. W.
name: Kirkpatrick, J. Davy
name: McElwain, M. W.
name: Bonaventura, N. R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Keck near-infrared imaging of three binary L dwarf systems, all of which are likely to be sub-stellar. Two are lithium dwarfs, and a third exhibits an L7 spectral type, making it the coolest binary known to date. All have component flux ratios near 1 and projected physical separations between 5 and 10 AU, assuming distances of 18 to 26 pc from recent measurements of trigonometric parallax. These surprisingly similar binaries represent the sole detections of companions in ten L dwarf systems which were analyzed in the preliminary phase of a much larger dual-epoch imaging survey. The detection rate prompts us to speculate that binary companions to L dwarfs are common, that similar-mass systems predominate, and that their distribution peaks at radial distances in accord both with M dwarf binaries and with the radial location of Jovian planets in our own solar system. To fully establish these conjectures against doubts raised by biases inherent in this small preliminary survey, however, will require quantitative analysis of a larger volume-limited sample which has been observed with high resolution and dynamic range.
description: LaTex manuscript in 13 pages, 3 postscript figures, Accepted for publication in the Letters of the Astrophysical Journal; Postscript pre-print version available at: http://www.hep.upenn.edu/PORG/papers/koerner99a.ps
VLBA Absorption Imaging of Ionized Gas Associated with the Accretion Disk in NGC 1275
Creators: name: Walker, R. C.
name: Dhawan, V.
name: Romney, J. D.
name: Kellermann, K. I.
name: Vermeulen, R. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Nearly simultaneous VLBA observations of 3C 84, the radio source associated with NGC 1275, have been made at multiple frequencies to study the free-free absorption of the northern, or "counterjet", feature found by Walker, Romney, and Benson (1994, Ap.J. 430, L45) and by Vermeulen, Readhead, and Backer (1994, Ap.J. 430, L41). Our observations confirm that the spectra are consistent with free-free absorption and eliminate the possibility that the earlier result was an effect of variability. The northern feature is well resolved spatially, so images have been made showing the distribution of the absorption over a region of about 1.5 pc on a side, beginning about 1.5 pc from the presumed location of the central object. That distribution is dominated by a strong decrease with radial distance. The magnitude of the absoption near 2.5 pc projected distance from the central object is consistent with a 10^4 K gas with an emission measure of about 5 X 10^8 pc cm^-6. The geometry is consistent with absorption by ionized gas associated with an accretion disk. The data provide firm constraints for models of the outer regions of accretion disks and, perhaps, associated winds.
description: 24 pages, 9 figures. Accepted 1999 Sept. 9 for publication in the Astrophysical Journal
Sertularia avicularia Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia avicularia

description: Sertularia avicularia [spec. nov.]
S. denticulis suboppositis mucronatis, calycibus globosis mucronatisque sessilibus, ramis dichotomis.
Ellis corall. 36. n. 2. t. 20. f. A. & t. 28. f. 7. Corallina cellifera erecta ramosa & plumosa sphaerulas testaceas summa parte aviumque capitum formas e latere cellularum gerens.
Habitat in Oceano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 809, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Charge sensitivity enhancement via mechanical oscillation in suspended carbon nanotube devices
Creators: name: Häkkinen, Pasi
name: Isacsson, Andreas
name: Savin, Alexander
name: Sulkko, Jaakko
name: Hakonen, Pertti
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Single electron transistors (SETs) fabricated from single-walled carbon nanotubes (SWNTs) can be operated as highly sensitive charge detectors reaching sensitivity levels comparable to metallic radio frequency SETs (rf-SETs). Here we demonstrate how the charge sensitivity of the device can be improved by using the mechanical oscillations of a single-walled carbon nanotube quantum dot. To optimize the charge sensitivity $δQ$, we drive the mechanical resonator far into the nonlinear regime and bias it to an operating point where the mechanical third order nonlinearity is cancelled out. This way we enhance $δQ$, from 6 $μe/\sqrt{\textrm{Hz}}$ for the static case, to 0.97 $μe/\sqrt{\textrm{Hz}}$, at a probe frequency of $\sim$ 1.3 kHz.
description: 8 pages + 12 page supplement
A Model for the Three Lepton Decay Mode of the Proton
Creators: name: Brahmachari, Biswajoy
name: O'Donnell, Patrick J.
name: Sarkar, Utpal
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: An extension of the left--right symmetric model has been constructed which gives in a natural way the three lepton decay modes of the proton which have been suggested as an explanation for the atmospheric neutrino anomaly. We write down the potential which after minimization gives the proper choice of the Higgs spectrum. With this Higgs spectrum we then study the evolution of the gauge coupling constants and point out that for consistency one has to include effects of gravity.
description: We have added a section discussing the question of numerical values of the different scales in the evolution of the coupling constants. The figure is included at the end of the paper
Modeling the inactivation kinetics of lactic acid bacteria in a spray dryer
Creators: name: Jin, Dongbiao
name: Mao, Houjuan
name: Xiao, Jie
name: Zhang, Huanhuan
name: Woo, Meng Wai
name: Chen, Xiao Dong
name: Fu, Nan
Publisher: name: Taylor & Francis
Year: 2023
Subjects: Biochemistry
Neuroscience
Environmental Sciences not elsewhere classified
Biological Sciences not elsewhere classified

description: Changes in the viability of probiotic cells during spray drying were tracked, by developing an inactivation model of Lactobacillus rhamnosus GG (LGG) and coupling the model to the drying kinetics of spray drying using Computational Fluid Dynamics simulation. Six inactivation models in the Arrhenius-equation form were developed using single droplet drying experiments with average drying rates of 0.011–0.044 kg/kg/s; all gave reliable goodness-of-fit. In simulating spray drying process, the predicted moisture content of LGG-containing particles well followed experimental trends. However, only inactivation model 6, which incorporated droplet temperature, moisture content, rate of temperature change, and drying rate, accurately predicted the survival of LGG. Models 1–5 that incorporated fewer kinetics parameters with higher activation energy values underestimated the degree of inactivation. The findings highlighted the crucial effects of the rates of temperature and moisture content change on the inactivation of probiotics during rapid drying with average drying rates of 0.31–0.81 kg/kg/s.
Boron neutrino flux and the MSW solution of the solar neutrino problem
Creators: name: Krastev, P. I.
name: Smirnov, A. Yu.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: There are large uncertainties in the predictions of the boron neutrino flux from the Sun which cannot be considered as being of purely statistical origin. We treat the magnitude of this flux, $Φ_B$, as a parameter to be found from experiment. The properties of the MSW solution to the solar neutrino problem for different values of $Φ_B$ are studied. Present data give the bounds: $0.38 < Φ_B/ Φ_B^0 < 3.1$ (2$σ$), where $Φ_B^0 \equiv 5.7 \cdot 10^6$ cm$^{-2}$s$^{-1}$ is the flux in the reference SSM. The variations of the flux in this interval enlarge the allowed region of mixing angles: $\sin^2 2θ= 8\cdot 10^{-4} ÷2\cdot 10^{-2}$ (small mixing solutions) and $\sin^2 2θ= 0.2 ÷0.85$ (large mixing solution). If the value of the original boron neutrino flux is about that measured by Kamiokande, a consistent description of the data is achieved for $\sin^2 2θ\sim (0.8 ÷2)\cdot 10^{-3}$ (``very small mixing solution"). The solution is characterized by a strong suppression of the beryllium neutrino line, a weak distortion of the high energy part of the boron neutrino spectrum and a value of the double ratio $(CC/NC)^{exp}/(CC/NC)^{SSM}$ at $E > 5$ MeV close to 1. We comment on the possibility to measure the neutrino parameters and the original boron neutrino flux in future experiments.
description: 16 pages + 3 figures (4 uuencoded postscript files), DOE/ER/40561-137-INT94-13-02
Additional file 6: of Modeling of the GC content of the substituted bases in bacterial core genomes
Creators: name: Bohlin, Jon
name: Eldholm, Vegard
name: Brynildsrud, Ola
name: Petterson, John
name: Alfsnes, Kristian
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 60506 Virology

description: The figure shows the difference between bulk sbGC and corresponding cgGC (i.e. cgGC subtracted from sbGC) plotted against cgGC (horizontal axis) as well as the estimated values from (gcMOD-cgGC) (blue line). (PDF 8Â kb)
A Mid-Infrared and Far-Infrared View of Galaxies
Creators: name: Cesarsky, C. J.
name: Sauvage, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: From the disk of normal galaxies to the nucleus of prototype active sources, we review the wealth of results and new understanding provided by recent infrared probes and, in particular, the four instruments on-board of ISO.
description: Review presented at the Millenium Conference on Galaxy Morphology (D. Block, I. Puerari, A. Stockton, dW. Ferreira Eds), Johannesburg, South Africa. 18 pages, 4 figures (fig3 is provided in gif to cut on size, should be converted to postscript). Includes the kluwer style files
Sertularia rugosa Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia rugosa

description: Sertularia rugosa [spec. nov.]
S. denticulis alternis obsoletis, calycibus rugosissimis, ramis vagis.
Ellis corall. 26. n. 23. t. 15. f. A. Corallina exigua repens, denticulis alternis, fructus medicae cochleatae aemulis.
Habitat in Oceano.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 809, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Multiplicity Functions and X-ray emission of Clusters and Groups versus Galaxies and Quasars
Creators: name: Valageas, P.
name: Schaeffer, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a unified analytical formulation for the multiplicity functions of clusters and galaxies which is free from the cloud-in-cloud problem encountered in earlier approaches and well adapted to the description of the non-linear clustering features. It is especially suited to simultaneously describe rich clusters, groups and galaxies, consistently with the hierarchical picture of gravitational clustering and their evolution in time. Using a simple model for the X-ray luminosity (taking into account entropy considerations), we obtain the X-ray luminosity distribution of groups and clusters. Then, using the same formalism we derive the galaxy and quasar multiplicity functions. In particular, we show that the use of the standard Press-Schechter prescription leads to erroneous conclusions at low redshifts while our approach provides a reasonable agreement with observations in a natural fashion because it is able to distinguish galactic halos from groups or clusters. Thus, we obtain a global and consistent picture of the X-ray emissions from all structures. In particular, we show that future observations (e.g., from AXAF) could provide interesting information on galaxy evolution. Indeed, they will constrain the importance of a possible hot diffuse gaseous phase in galactic halos and they could reveal massive galaxies which are just being formed, through the X-ray emission of their cooling gas.
description: 23 pages, final version published in A&A. Improved modeling of the temperature - X-ray luminosity relation for clusters. More detailed discussion of the need to properly distinguish galactic halos from simple "just-virialized" objects in order to draw meaningful conclusions for the luminosity functions of galaxies and QSOs
Heusler, Weyl, and Berry
Creators: name: Manna, Kaustuv
name: Sun, Yan
name: Müchler, Lukas
name: Kübler, Jürgen
name: Felser, Claudia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Heusler materials, initially discovered by Fritz Heusler more than a century ago, have grown into a family of more than 1000 compounds, synthesized from combinations of more than 40 elements. These materials show a wide range of properties, but new properties are constantly being found. Most recently, by incorporating heavy elements that can give rise to strong spin-orbit coupling (SOC), non-trivial topological phases of matter, such as topological insulators (TIs), have been discovered in Heusler materials. Moreover, the interplay of symmetry, SOC and magnetic structure allows for the realization of a wide variety of topological phases through Berry curvature design. Weyl points and nodal lines can be manipulated by various external perturbations, which results in exotic properties such as the chiral anomaly, and large anomalous spin and topological Hall effects. The combination of a non-collinear magnetic structure and Berry curvature gives rise a non-zero anomalous Hall effect, which was first observed in the antiferromagnets Mn3Sn and Mn3Ge. Besides this k-space Berry curvature, Heusler compounds with non-collinear magnetic structures also possess real-space topological states in the form of magnetic antiskyrmions, which have not yet been observed in other materials. The possibility of directly manipulating the Berry curvature shows the importance of understanding both the electronic and magnetic structures of Heusler compounds. Together, with the new topological viewpoint and the high tunability, novel physical properties and phenomena await discovery in Heusler compounds.
description: 24 pages, 5 figures
German Spelling Measure
Creators: name: Haase, Astrid
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Education
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: Morphological Spelling Measure

description: In this self-constructed spelling measure, participants write 25 irregular German words.
The target words are all intransparent. This means, they contain at least one grapheme (a letter or several letters that represent one sound, e.g. a, th) that are spelled incorrectly if phoneme-grapheme-correspondence rules are used, but are spelled correctly if a morphological spelling strategy is used.
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000747
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Châtelet
subject: registre
subject: LaMOP

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1000747
Tevatron and LEP-II Probes of Minimal and String-Motivated Supergravity Models
Creators: name: Baer, H.
name: Gunion, J. F.
name: Kao, C.
name: Pois, H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We explore the ability of the Tevatron to probe Minimal Supersymmetry with high energy scale boundary conditions motivated by supersymmetry breaking in the context of supergravity/superstring theory. A number of boundary condition possibilities are considered: dilaton-like string boundary conditions applied at the standard GUT unification scale or alternatively at the string scale; and extreme (``no-scale'') minimal supergravity boundary conditions imposed at the GUT scale or string scale. For numerous specific cases within each scenario the sparticle spectra are computed and then fed into ISAJET 7.07 so that explicit signatures can be examined in detail. We find that, for some of the boundary condition choices, large regions of parameter space can be explored via same-sign dilepton and isolated trilepton signals. For other choices, the mass reach of Tevatron collider experiments is much more limited. We also compare mass reach of Tevatron experiments with the corresponding reach at LEP 200.
description: 44 pages, requires phyzzx.tex, tables.tex, full postscript file including embedded figures available via anonymous ftp at ucdhep.ucdavis.edu as [anonymous.gunion]bgkp.ps, preprint UCD-94-19
HST Observations of New Horizontal Branch Structures in the Globular Cluster omega Centauri
Creators: name: D'Cruz, Noella L.
name: O'Connell, Robert W.
name: Rood, Robert T.
name: Whitney, Jonathan H.
name: Dorman, Ben
name: Landsman, Wayne B.
name: Hill, Robert S.
name: Stecher, Theodore P.
name: Bohlin, Ralph C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The globular cluster omega Centauri contains the largest known population of very hot horizontal branch (HB) stars. We have used the Hubble Space Telescope to obtain a far-UV/optical color-magnitude diagram of three fields in omega Cen. We find that over 30% of the HB objects are ``extreme'' HB or hot post-HB stars. The hot HB stars are not concentrated toward the cluster center, which argues against a dynamical origin for them. A wide gap in the color distribution of the hot HB stars appears to correspond to gaps found earlier in several other clusters. This suggests a common mechanism, probably related to giant branch mass loss. The diagram contains a significant population of hot sub-HB stars, which we interpret as the ``blue-hook'' objects predicted by D'Cruz et al. (1996a). These are produced by late He-flashes in stars which have undergone unusually large giant branch mass loss. omega Cen has a well-known spread of metal abundance, and our observations are consistent with a giant branch mass loss efficiency which increases with metallicity.
description: Submitted to ApJ, 12 pages, including 3 figures, also available at http://www.physics.usyd.edu.au/~noella/research.html
Attosecond electronic recollision as field detector
Creators: name: Carpeggiani, P.
name: Reduzzi, M.
name: Comby, A.
name: Ahmadi, H.
name: Kühn, S.
name: Frassetto, F.
name: Poletto, L.
name: Hoff, D.
name: Ullrich, J.
name: Schröter, C. D.
name: Moshammer, R.
name: Paulus, G. G.
name: Sansone, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We demonstrate the complete reconstruction of the electric field of visible-infrared pulses with energy as low as a few tens of nanojoules. The technique allows for the reconstruction of the instantaneous electric field vector direction and magnitude, thus giving access to the characterisation of pulses with an arbitrary time-dependent polarisation state. The technique combines extreme ultraviolet interferometry with the generation of isolated attosecond pulses.
description: 5 figures
Vector-like Strong Coupling theory with small S and T parameters
Creators: name: Maekawa, Nobuhiro
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a mechanism which can reduce the Peskin and Takeuchi's S, T and U parameters in dynamical electroweak symmetry breaking models. It is interesting that not only S but also T parameter can become small even if there exists large isospin violation in fermion condensation. For example, when we take the $SU(2)_L\times U(1)_Y$ breaking mass of up-type fermion $m_U=1$ TeV and that of down-type $m_D=0$, we get S$\sim 0.001 N$ and T$\sim 0.05 N$ for the $SU(2)_L\times U(1)_Y$ invariant masses $M=10$ TeV. The point is that these parameters are suppressed by $SU(2)_L\times U(1)_Y$ invariant masses which the vector-like fermions can have.
Additional file 1: of Embolizing pulmonary aspergillosis, mycobacterial & aspergillous splenic abscess and cytomegalovirus co-infection following steroid induced immunosuppression: a case report
Creators: name: Harsha Dissanayake
name: Weeratunga, Praveen
name: Panduka Karunanayake
name: Rushika Lanerolle
name: M. Chandu De Silva
name: Jayasinghe, Saroj
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Timeline. Graphical representation of temporal evolution of the disease. (DOCX 38 kb)
Role of Scalar Meson Resonances in $K_{L}^{0} \rightarrow π^{0} γγDecay
Creators: name: Fajfer, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Corrections to $K_{L}^{0}\rightarrow π^{0} γγ$ decay induced by scalar meson exchange are studied within chiral perturbation theory. In spite of bad knowledge of scalar-mesons parameters, the calculated branching ratio can be changed by a few percent.
description: 18 pages of text, 2 figures (available upon request); preprint IJS-TP-16-94 , TUM-T31-63-94#
Microlensing towards different Galactic targets
Creators: name: Grenacher, Lukas
name: Jetzer, Philippe
name: Strässle, Marcus
name: De Paolis, Francesco
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculate the optical depth and the number of events due to gravitational microlensing towards the Galactic bulge, the spiral arm directions $γ$ Scutum, $β$ Scutum, $γ$ Normae, $\vartheta$ Muscae and some dwarf galaxies in the halo of the Galaxy. Using the events found by the MACHO collaboration during their first year of observation towards Baade's Window we estimate the mass functions for the bulge and disk populations following the mass moment method. We find that the mass function can be described by a decreasing power-law with slope $α\simeq 2.0$ in both cases and a minimal mass of $\sim 0.01$ $M_{\odot}$ for the bulge and $\sim 0.02$ $M_{\odot}$ for the disk, respectively. Assuming that the obtained mass function for the disk is also valid in the spiral arms, we find that the expected number of events towards the spiral arms is in reasonable agreement with the observations. However, the small number of observed events does not yet constrain much the different parameters entering in the computation of the mass function. To study the influence of the Magellanic Clouds on the shape and the velocity dispersion in the halo we perform a N-body simulation. We find that their presence induces a slight flattening of the halo ($q_{H}\simeq 0.8$). As a result the expected number of microlensing events towards some targets in the halo, such as the LMC or the SMC, decreases by about 20%, whereas due to the the modification induced on the velocity dispersion the event duration increases.
description: 13 pages, 8 figures, 2 reduced to low resolution, accepted for publication in A&A. A version with the high resolution figures can be found at ftp://www-theorie.physik.unizh.ch/pub/papers/1999092.ps.gz