cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Herniography - an investigation still in practice: A pictorial review
Creators: name: Bayam, Fatma
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: •We outline a simple and relatively safe technique for herniography and show examples of positive findings. •Potential complications are also...
MPEC 2024-L38 : 2024 LM
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 LM

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Nyctanthes hirsuta Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Oleaceae
Nyctanthes
Nyctanthes hirsuta

description: Nyctanthes hirsuta Linnaeus, Species Plantarum 1: 6. 1753.
"Habitat in India." RCN: 41.
Lectotype (Ridsdale in Manilal, Bot. Hist. Hort. Malab. 132. 1980): [icon] “Rava-pou” in Rheede, Hort. Malab. 4: 99, t. 48. 1683.
Current name: Nyctanthes hirsuta L. (Oleaceae).
Note: Green (in Kew Bull. 39: 653. 1984) discussed the name and its typification in some detail, but the type choice is attributable to an earlier account by Ridsdale.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 694, DOI: 10.5281/zenodo.291971
Structural and Dynamical Analysis of the Quiescent Molecular Ridge in the Large Magellanic Cloud
Creators: name: Finn, Molly K.
name: Indebetouw, Remy
name: Johnson, Kelsey E.
name: Costa, Allison H.
name: Chen, C. -H. Rosie
name: Kawamura, Akiko
name: Onishi, Toshikazu
name: Ott, Jürgen
name: Sewiło, Marta
name: Tokuda, Kazuki
name: Wong, Tony
name: Zahorecz, Sarolta
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a comparison of low-J 13CO and CS observations of four different regions in the LMC -- the quiescent Molecular Ridge, 30 Doradus, N159, and N113, all at a resolution of $\sim3$ pc. The regions 30 Dor, N159, and N113 are actively forming massive stars, while the Molecular Ridge is forming almost no massive stars, despite its large reservoir of molecular gas and proximity to N159 and 30 Dor. We segment the emission from each region into hierarchical structures using dendrograms and analyze the sizes, masses, and linewidths of these structures. We find that the Ridge has significantly lower kinetic energy at a given size scale and also lower surface densities than the other regions, resulting in higher virial parameters. This suggests that the Ridge is not forming massive stars as actively as the other regions because it has less dense gas and not because collapse is suppressed by excess kinetic energy. We also find that these physical conditions and energy balance vary significantly within the Ridge and that this variation appears only weakly correlated with distance from sites of massive star formation such as R136 in 30 Dor, which is $\sim1$ kpc away. These variations also show only a weak correlation with local star formation activity within the clouds.
description: 18 pages, 17 figures, accepted to AJ
title: Foreign bodies: A review of representative cases and a focus on magnetic resonance findings
Creators: name: Sousa, Marta
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To illustrate the spectrum of imaging findings resultant of foreign bodies (FB) on the several imaging modalities, namely radiography, ultrasound (US), computed tomography (CT), and magnetic resonance imaging(MRI). To discuss advantages and...
Reachability analysis of neural networks using mixed monotonicity
Creators: name: Meyer, Pierre-Jean
Publisher: name: arXiv
Year: 2021
Subjects: subject: Systems and Control (eess.SY)
subject: Machine Learning (cs.LG)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: This paper presents a new reachability analysis approach to compute interval over-approximations of the output set of feedforward neural networks with input uncertainty. We adapt to neural networks an existing mixed-monotonicity method for the reachability analysis of dynamical systems and apply it to each partial network within the main network. This ensures that the intersection of the obtained results is the tightest interval over-approximation of the output of each layer that can be obtained using mixed-monotonicity on any partial network decomposition. Unlike other tools in the literature focusing on small classes of piecewise-affine or monotone activation functions, the main strength of our approach is its generality: it can handle neural networks with any Lipschitz-continuous activation function. In addition, the simplicity of our framework allows users to very easily add unimplemented activation functions, by simply providing the function, its derivative and the global argmin and argmax of the derivative. Our algorithm is compared to five other interval-based tools (Interval Bound Propagation, ReluVal, Neurify, VeriNet, CROWN) on both existing benchmarks and two sets of small and large randomly generated networks for four activation functions (ReLU, TanH, ELU, SiLU).
title: The spectrum of gastrointestinal volvulus: twisting around the diagnosis
Creators: name: Gonçalves, Ligia
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: 1. To review the relevant anatomy for volvulus pathogenesis. 2. To describevolvulus’ mechanism and imaging featuresexemplifying with representative cases. 3. To discuss the crucial points in differential diagnosis making. 4. To emphasize the CT...
Jasminum sambac Aiton 1789
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Oleaceae
Jasminum
Jasminum sambac

description: Nyctanthes sambac Linnaeus, Species Plantarum 1:6. 1753.
"Habitat in India." RCN: 39.
Lectotype (Howard, Fl. Lesser Antilles 6: 83. 1989): Herb. Clifford: 5, Nyctanthes 1 (BM-000557517).
Current name: Jasminum sambac (L.) Aiton (Oleaceae).
Note: D’Arcy (in Ann. Missouri Bot. Gard. 63: 560. 1977) indicated 16.2 (LINN) as the type, but this is a Browne specimen received by Linnaeus only in 1758 and it is not original material for the name.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 694, DOI: 10.5281/zenodo.291971
HORuS transmission spectroscopy and revised planetary parameters of KELT-7b
Creators: name: Tabernero, H. M.
name: Osorio, M. R. Zapatero
name: Prieto, C. Allende
name: Gonzalez-Alvarez, E.
name: Sanz-Forcada, J.
name: Lopez-Gallifa, A.
name: Montes, D.
name: del Burgo, C.
name: Hernandez, J. I. Gonzalez
name: Rebolo, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report on the high-resolution spectroscopic observations of two planetary transits of the hot Jupiter KELT-7b ($M_{\rm p}$ $=$ 1.28 $\pm$ 0.17 M$_{\rm Jup}$, $T_{\rm eq}$ $=$ 2028 K) observed with the High Optical Resolution Spectrograph (HORuS) mounted on the 10.4-m Gran Telescopio Canarias (GTC). A new set of stellar parameters are obtained for the rapidly rotating parent star from the analysis of the spectra. Using the newly derived stellar mass and radius, and the planetary transit data of the Transiting Exoplanet Survey Satellite (TESS) together with the HORuS velocities and the photometric and spectroscopic data available in the literature, we update and improve the ephemeris of KELT-7b. Our results indicate that KELT-7 has an angle $λ$ = $-$10.55 $\pm$ 0.27 deg between the sky projections of the star's spin axis and the planet's orbital axis. By combining this angle and our newly derived stellar rotation period of 1.38 $\pm$ 0.05 d, we obtained a 3D obliquity $ψ$ = 12.4 $\pm$ 11.7 deg (or 167.6 deg), thus reinforcing that KELT-7 is a well-aligned planetary system. We search for the presence of H$α$, Li I, Na I, Mg I, and Ca II features in the transmission spectrum of KELT-7b but we are only able to determine upper limits of 0.08-1.4 % on their presence after accounting for the contribution of the stellar variability to the extracted planetary spectrum. We also discuss the impact of stellar variability in the planetary data. Our results reinforce the importance of monitoring the parent star when performing high-resolution transmission spectroscopy of the planetary atmosphere in the presence of stellar activity.
description: Accepted for publication in MNRAS
Model-Based Single Image Deep Dehazing
Creators: name: Li, Zhengguo
name: Zheng, Chaobing
name: Shu, Haiyan
name: Wu, Shiqian
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Model-based single image dehazing algorithms restore images with sharp edges and rich details at the expense of low PSNR values. Data-driven ones restore images with high PSNR values but with low contrast, and even some remaining haze. In this paper, a novel single image dehazing algorithm is introduced by fusing model-based and data-driven approaches. Both transmission map and atmospheric light are initialized by the model-based methods, and refined by deep learning approaches which form a neural augmentation. Haze-free images are restored by using the transmission map and atmospheric light. Experimental results indicate that the proposed algorithm can remove haze well from real-world and synthetic hazy images.
Anisotropic magnon damping by zero-temperature quantum fluctuations in ferromagnetic CrGeTe$_3$
Creators: name: Chen, Lebing
name: Mao, Chengjie
name: Chung, Jae-Ho
name: Stone, Matthew B.
name: Kolesnikov, Alexander I.
name: Wang, Xiaoping
name: Murai, Naoki
name: Gao, Bin
name: Delaire, Olivier
name: Dai, Pengcheng
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Spin and lattice are two fundamental degrees of freedom in a solid, and their fluctuations about the equilibrium values in a magnetic ordered crystalline lattice form quasiparticles termed magnons (spin waves) and phonons (lattice waves), respectively. In most materials with strong spin-lattice coupling (SLC), the interaction of spin and lattice induces energy gaps in the spin wave dispersion at the nominal intersections of magnon and phonon modes. Here we use neutron scattering to show that in the two-dimensional (2D) van der Waals honeycomb lattice ferromagnetic CrGeTe3, spin waves propagating within the 2D plane exhibit an anomalous dispersion, damping, and break-down of quasiparticle conservation, while magnons along the c axis behave as expected for a local moment ferromagnet. These results indicate the presence of dynamical SLC arising from the zero-temperature quantum fluctuations in CrGeTe3, suggesting that the observed in-plane spin waves are mixed spin and lattice quasiparticles fundamentally different from pure magnons and phonons.
description: 12 pages, 4 figures; Nature Communication in press
Sonnenfleckenzeichnung Nr. 243.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 05.10.1969, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Jasminum sambac Aiton 1789
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Oleaceae
Jasminum
Jasminum sambac

description: Nyctanthes undulata Linnaeus, Species Plantarum 1:6. 1753.
"Habitat in Malabaria." RCN: 40.
Lectotype (Green in Kew Bull. 58: 296. 2003): [icon] “Tsjiregammulla” in Rheede, Hort. Malab. 6: 97, t. 55. 1686.
Current name: Jasminum sambac (L.) Aiton (Oleaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 695, DOI: 10.5281/zenodo.291971
title: "Take an inch and it'll give a mile": A pictorial review of diaphragmatic hernias following esophagectomy with gastric pull-up or Nissen's fundoplication
Creators: name: Flanagan, Oisin
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To demonstrate the need to consider diaphragmatic hernia as a possible cause for obstructive bowel symptoms in patients following esophagectomy or Nissen’s Fundoplication. To show the benefit of multiplanar CT reconstruction for detection and...
title: Imaging features of small bowel and colorectal cancer in inflammatory bowel disease
Creators: name: Hristova, Lora
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To know the risk factors for developing small bowel cancer (SBC) and colorectal cancer (CRC) in patients with inflammatory bowel disease (IBD) •To know the clinical and pathological features of CRC and SBC in patients with IBD •To illustrate the...
Sonnenfleckenzeichnung Nr. 294.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.12.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Phase spirals in cosmological simulations of Milky Way-size galaxies
Creators: name: García-Conde, Begoña
name: Roca-Fàbrega, Santi
name: Antoja, Teresa
name: Ramos, Pau
name: Valenzuela, Octavio
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the vertical perturbations in the galactic disc of the Milky Way-size high-resolution hydrodynamical cosmological simulation named GARROTXA. We detect phase spirals in the vertical projection $Z- V_{Z}$ of disc's stellar particles for the first time in this type of simulations. Qualitatively similar structures were detected in the recent Gaia data, and their origin is still under study. In our model the spiral-like structures in the phase space are present in a wide range of times and locations across the disc. By accounting for an evolving mix of stellar populations, we observe that, as seen in the data, the phase spirals are better observed in the range of younger-intermediate star particles. We measure the intensity of the spiral with a Fourier decomposition and find that these structures appear stronger near satellite pericenters. Current dynamical models of the phase spiral considering a single perturber required a mass at least of the order of 10$^{10}$ M$_\odot$, but all three of our satellites have masses of the order of $\sim$10$^8$ M$_\odot$. We suggest that there are other mechanisms at play which appear naturally in our model such as the physics of gas, collective effect of multiple perturbers, and a dynamically cold population that is continuously renovated by the star formation Complementing collisionless isolated N-body models with the use of fully-cosmological simulations with enough resolution can provide new insights into the nature/origin of the phase spiral.
description: Updated several figures with reference system
Physical properties and trigonometric distance of the peculiar dwarf WISE J181005.5$-$101002.3
Creators: name: Lodieu, N.
name: Osorio, M. R. Zapatero
name: Martin, E. L.
name: Lopez, R. Rebolo
name: Gauza, B.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Our goal is to characterise the physical properties of the metal-poor brown dwarf population. In particular, we focus on the recently discovered peculiar dwarf WISE J1810055$-$1010023. We collected optical iz and near-infrared J-band imaging on multiple occasions over 1.5 years to derive accurate trigonometric parallax and proper motion of the metal-depleted ultra-cool dwarf candidate WISE1810. We also acquired low-resolution optical spectroscopy (0.6$-$1.0 $μ$m) and new infrared (0.9$-$1.3 $μ$m) spectra of WISE1810 that were combined with our photometry, other existing data from the literature and our trigonometric distance to determine the object's luminosity from the integration of the observed spectral energy distribution covering from 0.6 through 16$μ$m. We compared the full optical and infrared spectrum with state-of-the-art atmosphere models to further constrain its effective temperature, surface gravity and metallicity. WISE1810 is detected in the $iz$ bands with AB magnitudes of $i$=23.871$\pm$0.104 and $z$=20.147$\pm$0.083 mag in the PanSTARRS system. It does not show any obvious photometric variability beyond 0.1$-$0.2 mag in any of the $z$- and $J$-band filters. The very red $z-J \approx 2.9$ mag colour is compatible with an ultra-cool dwarf nature. Fitting for parallax and proper motion, we measure a trigonometric parallax of 112.5$^{+8.1}_{-8.0}$ mas for WISE1810, placing the object at only 8.9$^{+0.7}_{-0.6}$ pc, about three times closer than previously thought. We employed Monte Carlo methods to estimate the error on the parallax and proper motion. The object's luminosity was determined at log$L/L_\odot$=$-$5.78$\pm$0.11 dex. From the comparison to atmospheric models, we infer a likely metallicity of [Fe/H] $\approx -1.5$ and an effective temperature cooler than 1000K. Abridged
description: 12 pages, 15 figures, 6 tables, accepted for publications to A&A
Nymphaea alba Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Nymphaeales
Nymphaeaceae
Nymphaea
Nymphaea alba

description: Nymphaea alba Linnaeus, Species Plantarum 1: 510. 1753, typ. cons.
"Habitat in Europae & America aquis dulcibus." RCN: 3856.
Lectotype (Mitra in Nayar & al. in Fasc. Fl. India 20: 16. 1990): Herb. Linn. No. 673.4 (LINN).
Generitype of Nymphaea Linnaeus, nom. cons.
Current name: Nymphaea alba L. (Nymphaeaceae).
Note: Mitra’s choice of the material in LINN as type is unfortunate because detailed morphological and palynological studies show that it belongs not to N. alba but to N. Candida C. Presl & J. Presl (which Mitra recognised as a species distinct from N. alba). The two taxa are usually treated as distinct, though often at subspecific rank. Although Art. 57.1 provides some temporary protection for the name, a conservation proposal appears to be necessary.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 695, DOI: 10.5281/zenodo.291971
Unveiling the electron-nuclear spin dynamics in an n-doped InGaAs epilayer by spin noise spectroscopy
Creators: name: Rittmann, C.
name: Petrov, M. Yu.
name: Kamenskii, A. N.
name: Kavokin, K. V.
name: Kuntsevich, A. Yu.
name: Efimov, Yu. P.
name: Eliseev, S. A.
name: Bayer, M.
name: Greilich, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We discuss the implications of a small indium content (3%) in a GaAs epilayer on the electron- and nuclear-spin relaxation due to enhanced quadrupolar effects induced by the strain. Using the weakly perturbative spin-noise spectroscopy, we study the electron-spin relaxation dynamics without explicit excitation. The observed temperature dependence indicates the presence of localized states, which have an increased interaction with the surrounding nuclear spins. Time-resolved spin-noise spectroscopy is then applied to study the relaxation dynamics of the optically pumped nuclear-spin system. It shows a multi-exponential decay with time components, ranging from several seconds to hundreds of seconds. Further, we provide a measurement of the local magnetic field acting between the nuclear spins and discover a strong contribution of quadrupole effects. Finally, we apply the nuclear spin diffusion model, that allows us to estimate the concentration of the localized carrier states and to determine the nuclear spin diffusion constant characteristic for this system.
description: 13 pages, 9 figures
Theoretical model of external spinal cord stimulation
Creators: name: Shneider, Mikhail N.
name: Pekker, Mikhail
Publisher: name: arXiv
Year: 2021
Subjects: subject: Medical Physics (physics.med-ph)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: In this paper, a simple theoretical model of excitation of action potentials of multiple motor pools by stimulating current pulses over the lumbosacral regions of the spinal cord is presented. The present model is consistent with known experimental data.
Sonnenfleckenzeichnung Nr. 207.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.08.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Nymphaea lotus Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Nymphaeales
Nymphaeaceae
Nymphaea
Nymphaea lotus

description: Nymphaea lotus Linnaeus, Species Plantarum 1: 511. 1753.
"Habitat in calidis Indiae, Africae, Americae." RCN: 3857.
Lectotype (Verdcourt in Polhill, Fl. Trop. E. Africa, Nymphaeaceae: 3. 1989): [icon] "Lotus Aegyptia" in Alpino, Pl. Exot.: 214, 213. 1627.
Current name: Nymphaea lotus L. (Nymphaeaceae).
Note: Verdcourt (in Kew Bull. 44: 179. 20 Mar 1989) gave a detailed account but the typification dates from his slightly earlier (15 Feb 1989) Flora account.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 695, DOI: 10.5281/zenodo.291971
Rotating and vibrating symmetric top molecule RaOCH$_3$ in the fundamental $\mathcal{P}$, $\mathcal{T}$-violation searches
Creators: name: Zakharova, Anna
Publisher: name: arXiv
Year: 2021
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the influence of the rotations and vibrations of the symmetric top RaOCH$_3$ molecule on its effectiveness as a probe for the $\mathcal{P}$ and $\mathcal{T}$-violating effects, such as the electron electric dipole moment (eEDM) and the scalar-pseudoscalar electron-nucleon interaction (Ne-SPS). The corresponding enhancement parameters $E_{\rm eff}$ and $E_{\rm s}$ are computed for the ground and first excited rovibrational states with different values of the angular momentum component $K$. For the lowest $K$-doublet with $v_\perp=0$ and $K=1$ the values are $E_{\rm eff}=47.647\,\mathrm{GV/cm}$ and $E_{\rm s}=62.109\,\mathrm{kHz}$. The results show larger deviation from the equilibrium values than in triatomic molecules.
description: Equations (56) and (57) were corrected. Results for the Es and Eeff were improved
Nuphar lutea Sibth. & Sm.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Nymphaeales
Nymphaeaceae
Nuphar
Nuphar lutea

description: Nymphaea lutea Linnaeus, Species Plantarum 1: 510. 1753.
"Habitat in Europae littora sub dulci aqua." RCN: 3855.
Lectotype (Jonsell & Jarvis in Nordic J. Bot. 14: 159. 1994): Herb. Linn. No. 218 (LAPP), see p. 171.
Current name: Nuphar lutea (L.) Sibth. & Sm. (Nymphaeaceae).
Note: Beal (in J. Elisha Mitchell Sci. Soc. 72: 323. 1956) indicated material associated with genus 673 in LINN as the type, but there are three sheets (673.1, 673.2 and 673.3) associated with this name. As they are evidently not part of a single gathering, Art. 9.15 does not apply, and Jonsell & Jarvis’ type choice appears to be the earliest.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 695, DOI: 10.5281/zenodo.291971
Sonnenfleckenzeichnung Nr. 127.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 04.06.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
title: Spectrum of imaging appearances of abdominal desmoid disease complicating Familial Adenomatous Polyposis (FAP)
Creators: name: Dattani, Minaxi
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To demonstrate the differing degrees of hereditary desmoid disease and its related...
SpaceSaving$^\pm$: An Optimal Algorithm for Frequency Estimation and Frequent items in the Bounded Deletion Model
Creators: name: Zhao, Fuheng
name: Agrawal, Divyakant
name: Abbadi, Amr El
name: Metwally, Ahmed
Publisher: name: arXiv
Year: 2021
Subjects: subject: Databases (cs.DB)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences

description: In this paper, we propose the first deterministic algorithms to solve the frequency estimation and frequent item problems in the bounded deletion model. We establish the space lower bound for solving the deterministic frequent items problem in the bounded deletion model, and propose the Lazy SpaceSaving$^\pm$ and SpaceSaving$^\pm$ algorithms with optimal space bound. We then develop an efficient implementation of the SpaceSaving$^\pm$ algorithm that minimizes the latency of update operations using novel data structures. The experimental evaluations testify that SpaceSaving$^\pm$ has accurate frequency estimations and achieves very high recall and precision across different data distributions while using minimal space. Our analysis and experiments clearly demonstrate that SpaceSaving$^\pm$ provides more accurate estimations using the same space as the state of the art protocols for applications with up to 93% of items deleted. Moreover, motivated by prior work, we propose Dyadic SpaceSaving$^\pm$, the first deterministic quantile approximation sketch in the bounded deletion model.
title: Abdominal lymphoma: What radiologists need to know
Creators: name: Shin, YuRi
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: GI Tract - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: 1. To understand the lymphoma classification and staging system 2. To discuss how to compare and evaluate the CT and PET-CT findings for treatment response 3. To correlate between lymphoma subtypes and image findings 4. What image findings should...
Sonnenfleckenzeichnung Nr. 206.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 26.08.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Nelumbo nucifera Gaertn.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Proteales
Nelumbonaceae
Nelumbo
Nelumbo nucifera

description: Nymphaea nelumbo Linnaeus, Species Plantarum 1: 511. 1753.
"Habitat in Indiis." RCN: 3858.
Type not designated.
Original material: Herb. Hermann 3: 52, No. 193 (BM); Herb. Hermann 4: 69, No. 193 (BM); Herb. Hermann 5: 286, 287, No. 193 [icon] (BM); [icon] in Rheede, Hort. Malab. 11: 59, 61, t. 30, 31. 1692; [icon] in Plukenet, Phytographia: t. 207, f. 5. 1692; Almag. Bot.: 267. 1696.; [icon] in Plukenet, Phytographia: t. 322, f. 1. 1694; Almag. Bot.: 267. 1696.; [icon] in Hermann, Parad. Bat.: 205. 1698.
Current name: Nelumbo nucifera Gaertn. (Nelumbonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part N), pp. 690-695 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 695, DOI: 10.5281/zenodo.291971
title: Evaluation of hippocampal volume in patients with bipolar disorder comparing manual and automatic segmentation techniques
Creators: name: Döring, Thomas
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: The hippocampus is responsible for encoding emotionally relevant data into the declarative memory in the human brain (Bannerman et al., 2004; LaBar et al., 2006). Research suggests that the declarative memory processes of patients with bipolar...
Sonnenfleckenzeichnung Nr. 315.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.12.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Investigation of $^{11}$B and $^{40}$Ca levels at 8-9 MeV by Nuclear Resonance Fluorescence
Creators: name: Gribble, D.
name: Iliadis, C.
name: Janssens, R. V. F.
name: Friman-Gayer, U.
name: Krishichayan
name: Finch, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We report on the measurement of $^{11}$B and $^{40}$Ca levels between excitation energies of 8 and 9 MeV using nuclear resonance fluorescence (NRF). The experiment was carried out with nearly-monoenergetic and linearly polarized photon beams provided by the High-Intensity $γ$-ray Source (HI$γ$S) facility at the Triangle Universities Nuclear Laboratory (TUNL). States in $^{11}$B are important for calibrations of NRF measurements, while the properties of $^{40}$Ca levels impact potassium nucleosynthesis in globular clusters. For $^{40}$Ca, we report on improved excitation energies and an unambiguous $2^-$ assignment for the state at 8425 keV. For $^{11}$B, we obtained improved values for $γ$-ray multipolarity mixing ratios and branching ratios of the 8920 keV level.
description: 14 pages, 9 figures, to be published in Physical Review C
Probing light vector mediators with coherent scattering at future facilities
Creators: name: Bertuzzo, Enrico
name: di Cortona, Giovanni Grilli
name: Ramos, Lucas Magno D.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Future experiments dedicated to the detection of Coherent Elastic Neutrino-Nucleus Scattering may be powerful tools in probing light new physics. In this paper we study the sensitivity on light $Z'$ mediators of two proposed experiments: a directional low pressure Time Projection Chamber detector, $ν$BDX-DRIFT, that will utilize neutrinos produced at the Long Baseline Neutrino Facility, and several possible experiments to be installed at the European Spallation Source. We compare the results obtained with existing limits from fixed-target, accelerator, solar neutrino and reactor experiments. Furthermore, we show that these experiments have the potential to test unexplored regions that, in some case, could explain the anomalous magnetic moment of the muon or peculiar spectral features in the cosmic neutrino spectrum observed by IceCube.
description: 18 pages, 5 figures, 2 tables. Fixed a wrong sign in the NP contribution for the $L_{\mu}-L_{\tau}$ model in eq. 2.5 with respect to the previous version, updating related plots accordingly; the overall conclusions of the work have not changed
title: Efficient radiologic reading environment by using open-source AutoHotkey as connection software
Creators: name: Lee, Young Han
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Film-based radiology has been replaced by filmless radiology with Picture Archiving and Communicating System (PACS). Manually-written medical records and Prescription forms have changed by Hospital Information System (HIS) or Electric Medical Record...
Sonnenfleckenzeichnung Nr. 7.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.01.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
title: Diagnostic value of software-based-image-fusion of computed tomography and F18-FDG-PET scans in patients with cancer of unknown primary
Creators: name: Henninger, Benjamin
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: To evaluate the accuracy of software-based-image-fusion of 2-deoxy-2-[fluorine-18]fluoro-D-glucose (FDG) positron emission tomography (PET) and computed tomography (CT) in the imaging of patients with cancer of unknown primary...
title: Colon CAD: What the radiologists need to know
Creators: name: Ferrari, Riccardo
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To provide basic and advanced description of colon CAD software, concerning technical basis and principal pitfalls; to understand what are the benefits and the disadvantages of using it in the clinical workflow; to review results of the most recent...
Quasars as high-redshift standard candles
Creators: name: Sacchi, A.
name: Risaliti, G.
name: Signorini, M.
name: Lusso, E.
name: Nardini, E.
name: Bargiacchi, G.
name: Bisogni, S.
name: Civano, F.
name: Elvis, M.
name: Fabbiano, G.
name: Gilli, R.
name: Trefoloni, B.
name: Vignali, C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The non-linear relation between the X-ray and ultraviolet (UV) luminosity in quasars has been used to derive quasar distances and to build a Hubble diagram at redshifts up to $z\sim$ 7. This cosmological application is based on the assumption of independence of the relation on redshift and luminosity. We want to test the reliability of this hypothesis by studying the spectroscopic properties of high-redshift quasars in the X-ray and UV bands. We performed a one-by-one analysis of a sample of 130 quasars at $z>$ 2.5 with high-quality X-ray and UV spectroscopic observations. We found that not only the X-ray to UV correlation still holds at these redshifts, but its intrinsic dispersion is as low as 0.12 dex (previous works reached 0.20$-$0.22 dex). For a sample of quasars at $z\sim$ 3 with particularly high-quality observations the dispersion further drops to 0.09 dex, a value entirely accountable for by intrinsic variability and source geometry effects. The composite spectra of these quasars, in both the X-rays and the UV, do not show any difference with respect to the average spectra of quasars at lower redshifts. The absence of any spectral difference between high- and low-$z$ quasars and the tightness of the X-ray to UV relation suggests that no evolutionary effects are present in the relation. Therefore, it can be safely employed to derive quasar distances. Under this assumption, we obtain a measurement of the luminosity distance at $z\sim$ 3 with 15 % uncertainty, and in a 4$σ$ tension with the concordance model.
description: Accepted for publication in Astronomy & Astrophysics Letters, 8 pages, 6 figures
Sonnenfleckenzeichnung Nr. 260.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 22.10.1969, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Low-energy excitations and magnetic anisotropy of the layered van der Waals antiferromagnet Ni$_2$P$_2$S$_6$
Creators: name: Mehlawat, K.
name: Alfonsov, A.
name: Selter, S.
name: Shemerliuk, Y.
name: Aswartham, S.
name: Büchner, B.
name: Kataev, V.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The quasi-two-dimensional antiferromagnet Ni$_2$P$_2$S$_6$ belongs to the family of magnetic van der Waals compounds that provides a rich material base for the realization of fundamental models of quantum magnetism in low dimensions. Here, we report high-frequency/high-magnetic field electron spin resonance measurements on single crystals of Ni$_2$P$_2$S$_6$. The results enable one to reliably determine the positive, "easy"-plane type of the single ion anisotropy of the Ni$^{2+}$ ions with the upper limit of its magnitude $\lesssim 0.7$ meV. The resonance response reveals strongly anisotropic spin fluctuations setting in shortly above the Néel temperature $T_{\rm N} = 158$ K and extending in the antiferromagnetically ordered state down to low temperatures. There, a low-energy magnon excitation gapped from the ground state by only $\sim 1$ meV was found. This magnon mode may explain unusual low temperature relaxation processes observed in a latest nuclear magnetic resonance experiments and together with the estimate of the single ion anisotropy they should enable setting up a realistic spin model for an accurate description of magnetic properties of Ni$_2$P$_2$S$_6$.
Sonnenfleckenzeichnung Nr. 246.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 08.10.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
Sonnenfleckenzeichnung Nr. 188.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 08.08.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
APPROACHES TO THE DEFINITION OF "RATIONALITY": REPRESENTATIONALISM VS. ENACTIVISM
Creators: name: Kryvitchenko, O.
Publisher: name: Zenodo
Year: 2022

description: Representationalists like M. Tay and S. Shoemaker adhere to the traditional philosophical view of rationality and distinguish two types — practical and epistemological. An epistemologically rational person is capable of reasoning, reviewing the bases of his reasoning with the advent of new data, and establishing the truth or falsity of their own beliefs. A practically rational person can act reasonably and consistently; however, practical rationality is subordinated to epistemological. This division is also supported by classical cognitive science: rationality prevails at the level of cognitive abilities, which appear as the operation of mental representations (i.e., propositional knowledge). At the same time, according to this definition, perceptual states are not rational; at the level of perception, there is only the fixation of sensory data ("raw data"). This step is understandable: if we recognized that perception is rational, then all beings who do not know the language, the rules of inference of propositional knowledge — animals, infants, wouldn't be able to perceive (which is not true).
Sonnenfleckenzeichnung Nr. 11.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 12.01.1969, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert