cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Non-traumatic chest in the emergency room
Creators: name: Costa, João
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Lung
subject: Respiratory system
subject: Thorax
subject: Chest - Miscellaneous

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: The major teaching points of this exhibit are: 1) To recognize the characteristic imaging findings associated with the most frequent conditions presenting with acute thoracic pain. 2) To provide a structured framework for developing a differential...
A census of young stellar objects in two line-of-sight star forming regions toward IRAS 22147+5948 in the outer Galaxy
Creators: name: Karska, Agata
name: Koprowski, Maciej
name: Solarz, Aleksandra
name: Szczerba, Ryszard
name: Sewiło, Marta
name: Siódmiak, Natasza
name: Elia, Davide
name: Gawroński, Marcin
name: Grzesiak, Konrad
name: Yung, Bosco H. K.
name: Fischer, William J.
name: Kristensen, Lars E.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: (abridged) Star formation in the outer Galaxy, i.e., outside of the Solar circle, has been lightly studied in part due to low CO brightness of molecular clouds linked with the negative metallicity gradient. Recent infrared surveys provide an overview of dust emission in large sections of the Galaxy, but suffer from cloud confusion and poor spatial resolution at far-infrared wavelengths. We aim to develop a methodology to identify and classify young stellar objects (YSOs) in star-forming regions in the outer Galaxy, and use it to solve a long-standing confusion with the distance and evolutionary status of IRAS 22147+5948. We use Support Vector Machine learning algorithm to complement standard color-color and color-magnitude diagrams in search for YSOs in the IRAS 22147 region using publicly available data from the `Spitzer Mapping of the Outer Galaxy' survey. The agglomerative hierarchical clustering algorithm is used to identify clusters, along with the Robitaille et al. (2017) code to calculate physical properties of individual YSOs. We identify 13 Class I and 13 Class II YSO candidates using the color-color diagrams, and additional 2 and 21 sources, respectively, using the machine learning techniques. Spectral energy distributions of 23 sources are modelled with a star and a passive disk, corresponding to Class II objects. Models of 3 sources include envelopes typical for Class I objects. The objects are grouped in 2 clusters located at the distance of ~2.2 kpc, and 5 clusters at ~5.6 kpc. The spatial extent of CO, radio continuum, and dust emission confirms the origin of YSOs in two distinct star-forming regions along a similar line-of-sight. The outer Galaxy might serve as a unique laboratory of star formation across environments on condition that complementary methods and ancillary data are used to properly account for cloud confusion and distance uncertainties.
description: 29 pages, 17 figures, 9 tables
Total absorption $γ$-ray spectroscopy of the $β$ decays of $^{96\text{gs,m}}$Y
Creators: name: Guadilla, V.
name: Meur, L. Le
name: Fallot, M.
name: Briz, J. A.
name: Estienne, M.
name: Giot, L.
name: Porta, A.
name: Cucoanes, A.
name: Shiba, T.
name: Zakari-Issoufou, A. -A.
name: Algora, A.
name: Tain, J. L.
name: Agramunt, J.
name: Jordan, D.
name: Monserrate, M.
name: Montaner-Pizá, A.
name: Nácher, E.
name: Orrigo, S. E. A.
name: Rubio, B.
name: Valencia, E.
name: Äystö, J.
name: Eronen, T.
name: Gorelov, D.
name: Hakala, J.
name: Jokinen, A.
name: Kankainen, A.
name: Kolhinen, V.
name: Koponen, J.
name: Moore, I.
name: Penttilä, H.
name: Pohjalainen, I.
name: Reinikainen, J.
name: Reponen, M.
name: Rinta-Antila, S.
name: Rytkönen, K.
name: Sonnenschein, V.
name: Voss, A.
name: Fraile, L. M.
name: Vedia, V.
name: Ganioğlu, E.
name: Gelletly, W.
name: Lebois, M.
name: Wilson, J. N.
name: Martinez, T.
name: Sonzogni, A. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The $β$ decays of the ground state (gs) and isomeric state (m) of $^{96}$Y have been studied with the total absorption $γ$-ray spectroscopy technique at the Ion Guide Isotope Separator On-Line facility. The separation of the 8$^{+}$ isomeric state from the 0$^{-}$ ground state was achieved thanks to the purification capabilities of the JYFLTRAP double Penning trap system. The $β$-intensity distributions of both decays have been independently determined. In the analyses the de-excitation of the 1581.6 keV level in $^{96}$Zr, in which conversion electron emission competes with pair production, has been carefully considered and found to have significant impact on the $β$-detector efficiency, influencing the $β$-intensity distribution obtained. Our results for $^{96\text{gs}}$Y (0$^+$) confirm the large ground state to ground state $β$-intensity probability, although a slightly larger value than reported in previous studies was obtained, amounting to $96.6_{-2.1}^{+0.3}\%$ of the total $β$ intensity. Given that the decay of $^{96\text{gs}}$Y is the second most important contributor to the reactor antineutrino spectrum between 5 and 7 MeV, the impact of the present results on reactor antineutrino summation calculations has been evaluated. In the decay of $^{96\text{m}}$Y (8$^{+}$), previously undetected $β$ intensity in transitions to states above 6 MeV has been observed. This shows the importance of total absorption $γ$-ray spectroscopy measurements of $β$ decays with highly fragmented de-excitation patterns. $^{96\text{m}}$Y (8$^{+}$) is a major contributor to reactor decay heat in uranium-plutonium and thorium-uranium fuels around 10 s after fission pulses, and the newly measured average $β$ and $γ$ energies differ significantly from the previous values in evaluated databases (...)
title: High-resolution transabdominal ultrasonography in identifying and characterizing duodenal and peri duodenal lesions
Creators: name: Hussain, Majaz
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: To evaluate the accuracy of high-resolution transabdominal ultrasonography (TAUS) in identifying and characterizing duodenal and peri duodenal lesions previously detected by endoscopy or other imaging...
Dust evolution with MUPPI in cosmological volumes
Creators: name: Parente, Massimiliano
name: Ragone-Figueroa, Cinthia
name: Granato, Gian Luigi
name: Borgani, Stefano
name: Murante, Giuseppe
name: Valentini, Milena
name: Bressan, Alessandro
name: Lapi, Andrea
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the evolution of dust in a cosmological volume using a hydrodynamical simulation in which the dust production is coupled with the MUPPI (MUlti Phase Particle Integrator) sub-resolution model of star formation and feedback. As for the latter, we keep as reference the model setup calibrated previously to match the general properties of Milky Way like galaxies in zoom-in simulations. However, we suggest that an increase of the star formation efficiency with the local dust to gas ratio would better reproduce the observed evolution of the cosmic star formation density. Moreover, the paucity of quenched galaxies at low redshift demands a stronger role of AGN feedback. We tune the parameters ruling direct dust production from evolved stars and accretion in the inter stellar medium to get scaling relations involving dust, stellar mass and metallicity in good agreement with observations. In low mass galaxies the accretion process is inefficient. As a consequence, they remain poorer in silicate and small grains than higher mass ones. We reproduce reasonably well the few available data on the radial distribution of dust outside the galactic region, supporting the assumption that the dust and gas dynamics are well coupled at galactic scales.
description: MNRAS accepted
title: Proliferation of measures contributes to advancing psychological science
Creators: name: Iliescu, Dragos
name: Greiff, Samuel
name: Ziegler, Matthias
name: Nye, Christopher
name: Geisinger, Kurt
name: Sellbom, Martin
name: Samuel, Douglas
name: Saklofske, Donald
Publisher: name: Humboldt-Universität zu Berlin
Year: 2024
Subjects: subject: Human behaviour
subject: 150 Psychologie

description: Proliferation and variability of psychological measures are part of the natural workings of the scientific process. They contribute to theory development, transparency, replicability, and validity, and restricting proliferation might hinder progress in the psychological sciences.
Sida hermaphrodita Rusby
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
Malvales
Malvaceae
Sida
Sida hermaphrodita

description: Napaea hermaphrodita Linnaeus, Species Plantarum 2: 686. 1753.
"Habitat in Virginia." RCN: 7518.
Replaced synonym of: Napaea laevis L. (1771), nom. illeg.
Lectotype (Iltis in Amer. Midi. Naturalist 70: 106. 1963): Herb. Linn. No. 1203.1 (LINN).
Current name: Sida hermaphrodita (L.) Rusby (Malvaceae).
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 690, DOI: 10.5281/zenodo.291971
Sonnenfleckenzeichnung Nr. 49.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 28.02.1971, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1971

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: Retrospective analysis of the relationship between periampullary duodenal diverticula and biliary disorders
Creators: name: Getsov, Plamen
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: The purpose of this retrospective analysis of the large population inBulgariawas to investigate the frequency of JPDD and its association with disorders of the biliary system in patients undergoing...
Sonnenfleckenzeichnung Nr. 309.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.12.1971, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1971

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: Women in fisheries management at Valencian Country’s Mediterranean Coast under an ecofeminist perspective
Creators: name: Mascarell, Yesmina
name: Herrera-Racionero, Paloma
Publisher: name: ASC 2015 - Theme session F
Year: 2024
Subjects: Technologies and data
Ecosystem observation, processes and dynamics

description: No abstracts are to be cited without prior reference to the author.Women in fisheries management at Valencian Country’s Mediterranean Coast under an ecofeminist perspective
The quarter median
Creators: name: Baringhaus, Ludwig
name: Grübel, Rudolf
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 62H12, 62H11, 62F35

description: We introduce and discuss a multivariate version of the classical median that is based on an equipartition property with respect to quarter spaces. These arise as pairwise intersections of the half-spaces associated with the coordinate hyperplanes of an orthogonal basis. We obtain results on existence, equivariance, and asymptotic normality.
Sonnenfleckenzeichnung Nr. 160.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.07.1971, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1971

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: Penetrating Crohn's disease: Correlation of CT enterography with surgical findings
Creators: name: Ballester, Gory
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: 1. To correlate the MDCT enterography (CTE) findings with the surgical findings in patients of penetrating Crohn’s disease (CD). 2. To understand the utility of MDCT enterography for the diagnosis and staging of penetrating Crohn’s...
Sonnenfleckenzeichnung Nr. 34.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 11.02.1971, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1971

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: Life history traits determine the shape and response to environmental conditions of a coastal community targeted by a Small-Scale Fishery
Creators: name: Fernández, Alexandre Alonso
name: Otero, Jaime
name: Díaz, Rafael Bañón
name: Álvarez, José Manuel Campelos
name: Fernández, Fernando Quintero
Publisher: name: ASC 2015 - Theme session F
Year: 2024
Subjects: Technologies and data
Ecosystem observation, processes and dynamics

description: No abstracts are to be cited without prior reference to the author.The understanding and prediction of the structure of marine communities from the environmental conditions they experience is a crucial yet elusive question in marine ecology. However, trait-based approaches in several fields have helped to understand the mechanisms underlying community assembly. Small-Scale Fisheries (SSFs) usually target coastal communities where a variety of species compose the catch. We used time series of standardized abundance for ten finfish species caught by the coastal NW Spain SSFs during 1999−2013 to test whether life history traits (LHTs) can explain community responses to environmental fluctuations. Time series were ordered using a principal component analysis. Species with smaller L-infinity and higher growth rate coefficient tended to have the highest relationship with the main trend found for the community. Moreover, those species were on average more variable and showed a stronger positive association with sea surface temperature over the preceding year. These results concur with ecological theory providing evidence that species with contrasting life histories perform differently to environmental conditions in an exploited fish community. This study provides support to the fact that on board collection of data helps to understand fish assemblage variation in SSFs.
title: Attention to the duodenum
Creators: name: Petrasova, Hana
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: 1. To describe normal anatomy and topographic relationships of the duodenum. 2. To remind and summarize radiologic findings in common and less frequent pathologic entities of the duodenum (congenital, inflammatory, traumatic, neoplastic...
Povĕst' o Sonečkĕ : Čast' vtoraja: Volodja
Creators: name: Cvetaeva, Marina
Publisher: name: [s.n.]
Year: 1937

description: Handschriftlicher Vermerk auf Bl. I
description: Marina Cvetaeva
description: Russisch
description: Verzeichnung=Description=Inventaire Oktober 2018 HAN-Katalogisierungsregeln
description: Digitalisierung=Digitization=Numérisation 06.09.2020 TIFF
description: 2 Originalverpackungen (Kartonmappe und -umschlag)
Galactic seismology: joint evolution of impact-triggered stellar and gaseous disc corrugations
Creators: name: Tepper-Garcia, Thor
name: Bland-Hawthorn, Joss
name: Freeman, Ken
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Evidence for wave-like corrugations are well established in the Milky Way and in nearby disc galaxies. These were originally detected as a displacement of the interstellar medium about the midplane, either in terms of vertical distance or vertical velocity. Over the past decade, similar patterns have emerged in the Milky Way's stellar disc. We investigate how these vertical waves are triggered by a passing satellite. Using high-resolution N-body/hydrodynamical simulations, we systematically study how the corrugations set up and evolve jointly in the stellar and gaseous discs. We find that the gas corrugations follow the stellar corrugations, i.e. they are initially in phase although, after a few rotation periods (500-700 Myr), the distinct waves separate and thereafter evolve in different ways. The spatial and kinematic amplitudes (and thus the energy) of the corrugations dampen with time, with the gaseous corrugation settling at a faster rate (~800 Myr versus ~1 Gyr). In contrast, the vertical energy of individual disc stars is fairly constant throughout the galaxy's evolution. This difference arises because corrugations are an emergent phenomenon supported by the collective, ordered motions of co-spatial ensembles of stars. We show that the damping of the stellar corrugations can be understood as a consequence of incomplete phase mixing, while the damping of the gaseous corrugations is a natural consequence of the dissipative nature of the gas. We suggest that - in the absence of further, strong perturbations - the degree of correlation between the stellar and gaseous waves may help to age-date the phenomenon.
description: MNRAS, in press. Title slightly shortened. References added. Matches accepted version
The GAPS programme at TNG XXXIV. Activity-rotation, flux-flux relationships, and active region evolution through stellar age
Creators: name: Maldonado, J.
name: Colombo, S.
name: Petralia, A.
name: Benatti, S.
name: Desidera, S.
name: Malavolta, L.
name: Lanza, A. F.
name: Damasso, M.
name: Micela, G.
name: Mallonn, M.
name: Messina, S.
name: Sozzetti, A.
name: Stelzer, B.
name: Biazzo, K.
name: Gratton, R.
name: Maggio, A.
name: Nardiello, D.
name: Scandariato, G.
name: Affer, L.
name: Baratella, M.
name: Claudi, R.
name: Molinari, E.
name: Bignamini, A.
name: Covino, E.
name: Pagano, I.
name: Piotto, G.
name: Poretti, E.
name: Cosentino, R.
name: Carleo, I.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Active region evolution plays an important role in the generation and variability of magnetic fields on the surface of lower main-sequence stars. However, determining the lifetime of active region growth and decay as well as their evolution is a complex task. We aim to test whether the lifetime for active region evolution shows any dependency on the stellar parameters. We identify a sample of stars with well-defined ages via their kinematics. We made use of high-resolution spectra to compute rotational velocities, activity levels, and emission excesses. We use these data to revisit the activity-rotation-age relationship. The time-series of the main optical activity indicators were analysed together with the available photometry by using Gaussian processes to model the stellar activity of these stars. Autocorrelation functions of the available photometry were also analysed. We use the derived lifetimes for active region evolution to search for correlations with the stellar age, the spectral type, and the level of activity. We also use the pooled variance technique to characterise the activity behaviour of our targets. Our analysis confirms the decline of activity and rotation as the star ages. We also confirm that the rotation rate decays with age more slowly for cooler stars and that, for a given age, cooler stars show higher levels of activity. We show that F- and G-type young stars also depart from the inactive stars in the flux-flux relationship. The gaussian process analysis of the different activity indicators does not seem to provide any useful information on active region's lifetime and evolution. On the other hand, active region's lifetimes derived from the light-curve analysis might correlate with the stellar age and temperature. Although we caution the small number statistics, our results suggest that active regions seem to live longer on younger, cooler, and more active stars.
description: Accepted by A&A
Sonnenfleckenzeichnung Nr. 234.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.09.1969, 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: Utility of MDCT enteroclysis in the evaluation of celiac disease and complications in adults
Creators: name: Tóth, Géza
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To show the usefulness of MDCT enteroclysis in the diagnosis of adult celiac disease. To show typical CT signs of celiac disease To show and to discuss complications of celiac...
Sida hermaphrodita Rusby
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
Malvales
Malvaceae
Sida
Sida hermaphrodita

description: Napaea laevis Linnaeus, Mantissa Plantarum Altera: 435. 1771, nom. illeg.
["Habitat in Virginia."] Sp. Pl. 2: 686 (1753). RCN: 7518.
Replaced synonym: Napaea hermaphrodita L. (1753).
Lectotype (Iltis in Amer. Midl. Naturalist 70: 106. 1963): Herb. Linn. No. 1203.1 (LINN).
Current name: Sida hermaphrodita (L.) Rusby (Malvaceae).
Note: A superfluous name for N. hermaphrodita L. (1753).
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 690, DOI: 10.5281/zenodo.291971
title: A gamut of magnetic resonance imaging findings in small bowel Crohn's disease
Creators: name: Gallego, Jose
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To illustrate the spectrum of MR findings in small bowel Crohn´s disease. To display a gamut of their typical appearances with MRI. To provide examples of endoscopic...
Sonnenfleckenzeichnung Nr. 20.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.01.1969, 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
Candidate eclipsing binary systems with a Delta Scuti star in Northern TESS field
Creators: name: Alicavus, F. Kahraman
name: Gumus, D.
name: Kirmizitas, O.
name: Ekinci, O.
name: Cavus, S.
name: Kaya, Y. T.
name: Alicavus, F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Existence of pulsating stars in eclipsing binaries has been known for decades. These types of objects are extremely valuable systems for astronomical studies as they exhibit both eclipsing and pulsation variations. The eclipsing binaries are the only way to directly measure the mass and radius of stars with a good accuracy ($\leq$1\%), while the pulsations are a unique way to probe the stellar interior via oscillation frequencies. There are different types of pulsating stars existing in eclipsing binaries. One of them is the Delta Scuti variables. Currently, the known number of Delta Scuti stars in eclipsing binaries is around 90 according to the latest catalog of these variables. An increasing number of these kinds of variables is important to understand the stellar structure, evolution and the effect of binarity on the pulsations. Therefore, in this study, we focus on discovering new eclipsing binaries with Delta Scuti component(s). We searched for the northern TESS field with a visual inspection by following some criteria such as light curve shape, the existence of pulsation like variations in the out-of-eclipse light curve and the Teff values of the targets. As a result of these criteria, we determined some targets. The TESS light curves of the selected targets first were removed from the binarity and frequency analysis was performed on the residuals. The luminosity, absolute and bolometric magnitudes of the targets were calculated as well. To find how much of these parameters represent the primary binary component (more luminous) we also computed the flux density ratio of the systems by utilizing the area of the eclipses. In addition, the positions of the systems in the H-R diagram were examined considering the flux density ratios. As a consequence of the investigation, we defined 38 candidates Delta Scuti and also one Maia variable in eclipsing binary systems.
title: MR small bowel enterography: Utility of dynamic imaging in the investigation of small bowel disease
Creators: name: Lloyd, Claire
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: Magnetic resonance (MR) imaging of the small bowel is gaining importance in the investigation of small bowel disease. We perform MR enterography and include a dynamic sequence in our protocol. This will be described and illustrated with case...
title: Challenges in minimizing illegal, unreported and unregulated (IUU) fishing of small-scale fisheries sector in Thailand
Creators: name: Suebpala, Wichin
name: Yeemin, Thamasak
name: Sutthacheep, Makamas
name: Chuenpagdee, Ratana
Publisher: name: ASC 2015 - Theme session F
Year: 2024
Subjects: Technologies and data
Ecosystem observation, processes and dynamics

description: No abstracts are to be cited without prior reference to the author.The sustainability of small-scale fisheries is highly linked on abundance of fishery resources and integrity of marine and coastal ecosystems. It is globally recognized that illegal, unreported and unregulated fishing (IUU) depletes fisheries resources, destroys important habitats, and further threaten to coastal fishing communities. In a context of small-scale fisheries, illegal fishing activities such as blast fishing and cyanide fishing etc. could be found in some areas especially in coral reefs and pinnacles. Some destructive fishing gears with a very small-mesh net are also modified and used without having proper measures and regulations. Currently, large number of small-scale fishing vessels have not been registered yet, while only small portion of small-scale fishers have official licenses to fish. Besides, catch data and other statistics as well as the understandings on ecological impacts from this sector poorly reported. However, relevant agencies have already started implementing some activities, for examples, the registration of small-scale fishing vessel and fishing licenses. Besides, the Fisheries Act B.E 2558 (2015) and Anti-Trafficking in Persons Act (No.2), B.E 2558 (2015) have also been official enforced in order to effectively support the management of IUU fishing in Thailand. Importantly, to overcome those challenges, collaboration among small-scale fishers, policy makers, and other stakeholders is highly required.
Identification of inertial modes in the solar convection zone
Creators: name: Triana, Santiago Andrés
name: Guerrero, Gustavo
name: Barik, Ankit
name: Rekier, Jérémy
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The observation of global acoustic waves (p modes) in the Sun has been key to unveiling its internal structure and dynamics. A different kind of wave, known as sectoral Rossby modes, have been observed and identified, which potentially opens the door to probing internal processes that are inaccessible through p mode helioseismology. Yet another set of waves, appearing as retrograde-propagating, equatorially antisymmetric vorticity waves, have also been observed but their identification remained elusive. Here, through a numerical model implemented as an eigenvalue problem, we provide evidence supporting the identification of those waves as a class of inertial eigenmodes, distinct from the Rossby mode class, with radial velocities comparable to the horizontal ones deep in the convective zone, but still small compared to the horizontal velocities towards the surface. We also suggest that the signature of tesseral-like Rossby modes might be present in the recent observational data.
description: 12 pages, 6 figures, accepted for publication in the Astrophysical Journal Letters
title: MDCT diagnostic performance evaluation in small bowel ischemia associated with obstruction
Creators: name: Zins, Marc
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Small bowel
subject: GI Tract - Small Bowel

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Small Bowel obstruction : The Key Role of the Radiologist - Small-bowel obstruction (SBO) is a commonly encountered finding at emergent abdominal CT, and the accuracy of CT in the diagnosis of moderate or severe bowel obstruction has been well...
Sonnenfleckenzeichnung Nr. 142.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.06.1971, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1971

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. 37.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.02.1971, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1971

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
Vertical distribution of cyclopropenylidene and propadiene in the atmosphere of Titan
Creators: name: Willacy, Karen
name: Chen, SiHe
name: Adams, Danica J.
name: Yung, Yuk L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Titan's atmosphere is a natural laboratory for exploring the photochemical synthesis of organic molecules. Significant recent advances in the study of the atmosphere of Titan include: (a) detection of C$_3$ molecules: C$_3$H$_6$, CH$_2$CCH$_2$, c-C$_3$H$_2$, and (b) retrieval of C$_6$H$_6$, which is formed primarily via C$_3$ chemistry, from Cassini-UVIS data. The detection of $c$-C$_3$H$_2$ is of particular significance since ring molecules are of great astrobiological importance. Using the Caltech/JPL KINETICS code, along with the best available photochemical rate coefficients and parameterized vertical transport, we are able to account for the recent observations. It is significant that ion chemistry, reminiscent of that in the interstellar medium, plays a major role in the production of c-C$_3$H$_2$ above 1000 km.
description: 18 pages (+ 27 page appendix), 16 figures
title: Diffusion-weighted MRI for parasternal staging in patients with primary breast cancer
Creators: name: Murata, Yoriko
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: MR
subject: Breast - MRI

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Parasternal staging in primary breast cancer is related to prognosis and greatly influences treatment strategy, but is typically defined by image assessment in primary breast cancer. Diffusion-weighted imaging (DWI) has recently become more...
Sonnenfleckenzeichnung Nr. 276.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 10.11.1969, 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. 299.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 11.12.1969, 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
title: Breast cancer in young women: Correlation between MRI features and pathological findings
Creators: name: Belli, Paolo
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: MR
subject: Breast - MRI

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: The aim of this study was to correlate Magnetic Resonance Imaging (MRI) features of breast cancer in young women with biological and hystopathological data. The reported incidence of breast cancer in women < 40 years of age is about 5-7% [1]....
THE CORRELATION BETWEEN INITIAL PIRANI SCORE AND NUMBER OF CASTS IN TREATMENT OF IDIOPATHIC CLUBFOOT BY PONSETI METHOD
Creators: name: Peshang Ibrahim Khudhur
name: Abdulkadr Muhammed Sleman Alany
name: Dedawan Namiq Rasul
Publisher: name: Zenodo
Year: 2024
Subjects: Idiopathic Clubfoot, Pirani Score, Casting, Ponseti Technique.

description: Abstract

Background: Clubfoot is a common congenital deformity of the lower limbs. It should be treated as soon as possible so that its correction is more easily achieved and the Ponseti method is the gold-standard treatment for idiopathic clubfeet, with good results reported globally. Materials and Method: The present study includes 44 children with clubfoot. All the patients were below the age of six months. The participants were treated by the technique of Ponseti methods and casting every week. The scoring of Pirani was used for the determination of deformity level. The scoring was done before and after the treatment. The Pirani score before and after the treatment was compared. Results: There were 68.18% male and 31.82% female patients in our study. There were unilateral 20 (45.45%) children while 24 (54.55%) patients with bilateral clubfoot. In our study, most of the cases (29 cases, 65.91%) were below one month of age. Forty-Three percent of the feet were corrected with fourth serial casting. The majority of the feet in the study had an initial Pirani score between 3 and 4. The range of Pirani score were 1.5-6, and around 8 (11.76%) feet in our study had the maximum Pirani score of ‘6’ Conclusion: The number of casts for correction in idiopathic Clubfoot is influenced by initial Pirani score. The repair of a club foot deformity using Ponseti's manipulation technique and casting has proven to be quite successful. After treatment, the majority of patients', Pirani scores showed excellent results.
Faster online calibration without randomization: interval forecasts and the power of two choices
Creators: name: Gupta, Chirag
name: Ramdas, Aaditya
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Data Structures and Algorithms (cs.DS)
subject: Computer Science and Game Theory (cs.GT)
subject: Methodology (stat.ME)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: We study the problem of making calibrated probabilistic forecasts for a binary sequence generated by an adversarial nature. Following the seminal paper of Foster and Vohra (1998), nature is often modeled as an adaptive adversary who sees all activity of the forecaster except the randomization that the forecaster may deploy. A number of papers have proposed randomized forecasting strategies that achieve an $ε$-calibration error rate of $O(1/\sqrt{T})$, which we prove is tight in general. On the other hand, it is well known that it is not possible to be calibrated without randomization, or if nature also sees the forecaster's randomization; in both cases the calibration error could be $Ω(1)$. Inspired by the equally seminal works on the "power of two choices" and imprecise probability theory, we study a small variant of the standard online calibration problem. The adversary gives the forecaster the option of making two nearby probabilistic forecasts, or equivalently an interval forecast of small width, and the endpoint closest to the revealed outcome is used to judge calibration. This power of two choices, or imprecise forecast, accords the forecaster with significant power -- we show that a faster $ε$-calibration rate of $O(1/T)$ can be achieved even without deploying any randomization.
description: 28 pages, published at Conference on Learning Theory (COLT) 2022
Sonnenfleckenzeichnung Nr. 48.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 02.03.1969, 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
Both the sun and the earth are fixed stars.pdf
Creators: name: Chen, Nuofu
Publisher: name: figshare
Year: 2022
Subjects: subject: 20199 Astronomical and Space Sciences not elsewhere classified
subject: FOS: Physical sciences

description: The heliocentric model has been widely accepted, so it is very difficult to believe that the heliocentric model has defects. However, there are two simple facts that show that the heliocentric model does have defects. There are two astronomical phenomena which cannot be explained with the heliocentric model. First astronomical phenomena, the direction of the Big Dipper observed on the earth is changing with the change of seasons. Second astronomical phenomena, there are always some stars that can be observed on the earth all year round. So, I try to use a new model to explain these two astronomical phenomena. The method I adopted is extremely simple, but to evaluate the correctness of this conclusion requires not only knowledge, but also courage.
Napaea dioica 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
Malvales
Malvaceae
Napaea
Napaea dioica

description: Napaea scabra Linnaeus, Mantissa Plantarum Altera: 435. 1771, nom. illeg.
["Habitat in Virginia."] Sp. Pl. 2: 686 (1753). RCN: 7519.
Replaced synonym: Napaea dioica L. (1753).
Lectotype (Iltis in Amer. Midi. Naturalist 70: 94. 1963): Herb. Linn. No. 1203.2 (LINN).
Current name: Napaea dioica L. (Malvaceae).
Note: A superfluous name for N. dioica L. (1753).
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 690, DOI: 10.5281/zenodo.291971
Sonnenfleckenzeichnung Nr. 9.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 10.01.1969, 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
New technique for determining a pulsar period: Waterfall principal component analysis
Creators: name: Cassanelli, Tomas
name: Naletto, Giampiero
name: Codogno, Giacomo
name: Barbieri, Cesare
name: Verroi, Enrico
name: Zampieri, Luca
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: This paper describes a new technique for determining the optimal period of a pulsar and consequently its light curve. The implemented technique makes use of the Principal Component Analysis (PCA) applied to the so-called waterfall diagram, which is a bidimensional representation of the pulsar acquired data. In this context we have developed the python package pywpf to easily retrieve the period with the presented method. We applied this technique to sets of data of the brightest pulsars in visible light that we obtained with the fast photon counter Iqueye. Our results are compared with those obtained by different and more classical analyses (e.g., epoch folding), showing that the periods so determined agree within the errors, and that the errors associated to the waterfall-PCA folding technique are slightly smaller than those obtained by the $χ^2$ epoch folding technique. We also simulated extremely noisy situations, showing that by means of a new merit function associated to the waterfall-PCA folding it is possible to get more confidence on the determined period with respect to the $χ^2$ epoch folding technique.
description: Accepted for publication by Astronomy & Astrophysics (A&A)