cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Sonnenfleckenzeichnung Nr. 120.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 28.05.1969, 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: MR guided large core biopsy versus MR guided vacuum assisted biopsy of breast lesions at 3T; Technical success rates and diagnostic yield
Creators: name: Mann, Ritse
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 increasing use of magnets with high field strength (3T and over) in clinical practice is eminent. There are suggestions that breast imaging at 3T has substantial advantages over imaging at 1.5T, including a higher diagnostic yield and a higher...
title: Use of molecular markers for monitoring the genetic effects of hatchery-basedstock enhancement and for tracking hatchery-born individuals in the great scallop (Pecten maximus)
Creators: name: Charrier, Grégory
name: Morvezen, Romain
name: Borcier, Elodie
name: Le Duff, Nolwen
name: Coheleach, Manon
name: Laroche, Jean
name: Boudry, Pierre
Publisher: name: ASC 2015 - Theme session I
Year: 2024
Subjects: Technologies and data
Pressures, impacts, conservation, and management

description: No abstracts are to be cited without prior reference to the author.The great scallop (Pecten maximus) is of high economical value, particularly in France and United-Kingdom. Although great scallop fisheries are mostly based on the exploitation of natural beds, somestocks are seeded with hatchery-reared spat in order to ensure the sustainability of local fisheries. Thisis particularly the case in the Bay of Brest (France), where hatchery-based stock enhancement of P.maximus has been developed since 1983, in order to enhance the local population. However, Therelease of hatchery-born seeds might significantly impact the genetic diversity of local scalloppopulations. In the present study, microsatellites were used to monitor the genetic variability seededgreat scallop populations, in order to evaluate the possible impact of hatchery-based stockenhancement on the genetic diversity of local populations. A limited but temporally persistent erosionof the genetic variability as well as a strong alteration of the natural gene pool were found in hatcherycohorts. However, the genetic diversity of seeded populations did not seem to decrease. Furthermore,molecular marker-based pedigrees were assessed, in order to identify hatchery-born individualsreleased in natural beds. Hatchery-born individuals were successfully assigned to their parents, thusopening new avenues for monitoring populations enhanced with hatchery-raised spat.
Discovery of recurrent flares of 6.7 GHz methanol maser emission in Cepheus A HW2
Creators: name: Durjasz, M.
name: Szymczak, M.
name: Olech, M.
name: Bartkiewicz, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context: Class II methanol masers at 6.7 GHz originate close to high-mass young stellar objects (HMYSOs). Their high sensitivity to local condition variations makes them a useful marker of the activity of the emerging massive stars. Aims: We aim to closely examine the variability of the 6.7 GHz methanol masers in Cep A HW2 using the new and archival single-dish and high-resolution Very-Long-Baseline Interferometry (VLBI) datasets. Methods: We monitored 6.7 GHz methanol masers towards the target between 2009 and 2021 using the Torun 32 m radio telescope, and analysed nine datasets of VLBI observations taken over 16 yr. Results: Faint, extremely redshifted maser emission located close to the presumed central star position and coincident with the radio jet shows flaring activity with a period of ~ 5 yr. Flares have an asymmetric profile with a rise-to-decay time ratio of 0.18 and relative amplitude higher than 10. The velocity of the flaring cloudlets drifts at a rate of 3-4 * 10^-5 km/s/d for about 11.5 yr of the monitoring. The time-lag between the peaks of the two flaring features implies a propagation speed of the exciting factor of ~ 1000 km/s. Synchronised and anticorrelated variations of the flux density of blue- and redshifted features begin ~ 2.5 yr after flares of the extremely redshifted emission.
description: 16 pages, 11 figures, 6 tables
title: Evaluation of breast tuberculosis: Spectrum of appearances on breast MRI
Creators: name: Jankharia, Bijal
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: To assess the modes of presentation and various imaging appearances of breast tuberculosis on MRI with a view to considering tuberculosis as a differential diagnosis while evaluating breast...
Evaluating Non-LTE Spectral Inversions with ALMA and IBIS
Creators: name: Hofmann, Ryan
name: Reardon, Kevin
name: Milic, Ivan
name: Molnar, Momchil
name: Chai, Yi
name: Uitenbroek, Han
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present observations of a solar plage in the millimeter-continuum with the ALMA and in the Ca 8542 and Na 5896 spectral lines with the Interferometric BIdimensional Spectrometer (IBIS). Our goal is to compare the measurement of local gas temperatures provided by ALMA with the temperature diagnostics provided by non-LTE inversions using STIC. In performing these inversions, we find that using column mass as the reference height scale, rather than optical depth, provides more reliable atmospheric profiles above the temperature minimum and that the treatment of non- LTE hydrogen ionization brings the inferred chromospheric temperatures into better agreement with the ALMA measurements. The Band 3 brightness temperatures are higher but well correlated with the inversion-derived temperatures at the height of formation of the Ca 8542 line core. The Band 6 temperatures instead do not show good correlations with the temperatures at any specific layer in the inverted atmospheres. We then performed inversions that included the millimeter continuum intensities as an additional constraint. Incorporating Band 3 generally resulted in atmospheres showing a strong temperature rise in the upper atmosphere, while including Band 6 led to significant regions of anomalously low temperatures at chromospheric heights. This is consistent with the idea that the Band 6 emission can come from a range of heights. The poor constraints on the chromospheric electron density with existing inversion codes introduces difficulties in determining the height(s) of formation of the millimeter continuum as well as uncertainties in the temperatures derived from the spectral lines.
description: 23 pages, 17 figures
Ctenium aromaticum Alph. Wood
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Ctenium
Ctenium aromaticum

description: Nardus gangitis Linnaeus, Species Plantarum 1: 53. 1753, nom. utique rej.
"Habitat in G. Narbonensi." RCN: 445.
Type not designated.
Original material: Herb. Linn. No. 73.6 (LINN); [icon] in Morison, Pl. Hist. Univ. 3: 257, s. 8, t. 13, f. penult., ult. 1699; [icon] in Plantin, Pl. Stirp. Icon.: 84. 1581.
Current name: Ctenium aromaticum (Walter) Alph. Wood (Poaceae).
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 692, DOI: 10.5281/zenodo.291971
CHARACTERISTICS OF PREGNANCY, CHILDBIRTH AND THE POSTPARTUM PERIOD IN PREGNANT WOMEN WITH AN ALLOGENEIC FETUS
Creators: name: N, Yesyp
Publisher: name: Zenodo
Year: 2022

description: Assisted reproductive technologies (ART) help to successfully overcome a number of aspects of such complex medical and social problems as infertility. In addition, the procedure of in vitro fertilization (IVF) using donor oocytes makes it possible to eliminate barriers caused by impaired gonadal development or premature loss of their function. However, it is known that patients enrolled in ART programs have an incidence of various obstetric and perinatal complications that differs from the general population, and both pathogenesis and actual rates are not yet known. It is obvious that the results of the use of ART with the formation of an allogeneic fetus are much less studied. The peculiarities of the fetoplacental complex functioning in such specific conditions and their impact on the incidence of obstetric and perinatal complications are not fully understood.
Sonnenfleckenzeichnung Nr. 106.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 12.05.1969, 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
Non-linear charged planar black holes in four-dimensional Scalar-Gauss-Bonnet theories
Creators: name: Bravo-Gaete, Moisés
name: Guajardo, Luis
name: Oliva, Julio
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work, we consider the recently proposed well-defined theory that permits a healthy $D\to 4$ limit of the Einstein-Gauss-Bonnet combination, which requires the addition of a scalar degree of freedom. We continue the construction of exact, hairy black hole solutions in this theory in the presence of matter sources, by considering a nonlinear electrodynamics source, constructed through the Plebański tensor and a precise structural function $\mathcal{H}(P)$. Computing the thermodynamic quantities with the Wald formalism, we identify a region in parameter space where the hairy black holes posses well-defined, non-vanishing, finite thermodynamic quantities, in spite of the relaxed asymptotic approach to planar AdS. We test its local stability under thermal and electrical fluctuations and we also show that a Smarr relation is satisfied for these black hole configurations.
description: 10 pages, 3 figures, Accepted for publication in Physical Review D
Sonnenfleckenzeichnung Nr. 203.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.08.1969, 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
Precision calculation of isospin-symmetry-breaking corrections to T=1/2 mirror decays using multi-reference charge-dependent density functional theory
Creators: name: Konieczka, M.
name: Bączyk, P.
name: Satuła, W.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present systematic study of isospin impurities ($α_{\rm ISB}$) to the wave functions of $T=1/2$, $11\leq A \leq 47$ mirror nuclei and the isospin-symmetry-breaking (ISB) corrections ($δ_{\rm ISB}^{\rm V}$) to their ground state vector $β$-decays using, for the first time, multi-reference charge-dependent density functional theory (MR-DFT) that includes strong-force-rooted class-III interaction adjusted to correct for the Nolen-Schiffer anomaly in nuclear masses. We demonstrate that, unexpectedly, the strong-force-rooted isovector force gives rise to a large systematic increase of $α_{\rm ISB}$ and $δ_{\rm ISB}^{\rm V}$ as compared to the results obtained within MR-DFT that uses Coulomb interaction as the only source of ISB. This, in turn, increases a central value of the $V_{\rm ud}$ element of the CKM matrix extracted from the $T=1/2$ mirrors bringing it closer to the value obtained form the purely vector superallowed $0^+ \to 0^+$ transitions. In order to compute the value of $V_{\rm ud}$, we performed precision calculation of the Fermi matrix elements in $A=19, 21, 35$, and 37 mirror nuclei using DFT-rooted configuration-interaction model that includes all relevant axially-deformed particle-hole configurations built upon Nilsson orbitals originating from the spherical $sd$ shell. Our calculations yield $|V_{\rm ud}|=0.9736(16)$.
description: 8 pages, 6 figures
Sonnenfleckenzeichnung Nr. 128.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.06.1969, 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
title: Ductal carcinoma in situ: Enhancement features on MR imaging
Creators: name: Luciani, Marialaura
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: To review the typical dynamic and morphological characteristics of Ductal Carcinoma in Situ (DCIS) on Magnetic Resonance Imaging...
Landau-Zener transitions through a pair of higher order exceptional points
Creators: name: Melanathuru, Rishindra
name: Malzard, Simon
name: Graefe, Eva-Maria
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Non-Hermitian quantum systems with explicit time dependence are of ever-increasing importance. There are only a handful of models that have been analytically studied in this context. Here, a PT-symmetric non-Hermitian $N$-level Landau-Zener type problem with two exceptional points of $N$th order is introduced. The system is Hermitian for asymptotically large times, far away from the exceptional points, and has purely imaginary eigenvalues between the exceptional points. The full Landau-Zener transition probabilities are derived, and found to show a characteristic binomial behaviour. In the adiabatic limit the final populations are given by the ratios of binomial coefficients. It is demonstrated how this behaviour can be understood on the basis of adiabatic analysis, despite the breakdown of adiabaticity that is often associated with non-Hermitian systems.
description: 12 pages, 5 figures
title: Population structure and genetic management unit delineation in the bluefin tuna using a genotyping-by-sequencing approach
Creators: name: Puncher, Gregory Neils
name: Cariani, Alessia
name: Maes, Gregory E.
name: Van Houdt, Jeroen
name: Herten, Koen
name: Albaina, Aitor
name: Cannas, Rita
name: Rodríguez-Ezpeleta, Naiara
name: Arrizabalaga, Haritz
name: Tinti, Fausto
Publisher: name: ASC 2015 - Theme session I
Year: 2024
Subjects: Technologies and data
Pressures, impacts, conservation, and management

description: No abstracts are to be cited without prior reference to the author.A genotyping-by-sequencing approach was to used to detect single nucleotide polymorphisms (SNPs) throughout the Atlantic bluefin tuna (BFT; Thunnus thynnus) genome while simultaneously analyzing the species' population structuring using 723 individuals captured between 2007-2013 from fourteen locations throughout the species' range. Due to the lack of an existing reference genome and sub-optimal performance of the restriction enzyme used (ApeKI), a novel data analysis approach was developed. By pooling the data from all individuals within geographic sampling locations, allele read count frequencies were calculated and compared. From a pool of 184,895 candidate SNPs, a high performance 96 SNP genotyping panel was developed in silico by selecting loci with pronounced differences in read count frequencies among young fish (larvae and young-of-the-year). Genotyping results revealed significant differentiation of samples from the Gulf of Mexico and Mediterranean (FST = 0.013). The composition of five mixed feeding aggregations in the Atlantic Ocean was determined via population assignment analysis of 230 adult fish. Our results provide evidence of persistent population structuring across broad geographic areas and can be used to estimate mixing rates, and with further development, may lead to traceability tools.
title: Contrast-enhanced magnetic resonance mammography (MRM): Improvement in breast lesion detection and characterization with gadobenate dimeglumine (Gd-BOPTA) compared to gadopentate dimeglumine (Gd-DTPA)
Creators: name: Pediconi, Federica
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: To prospectively and intra-individually compare equivalent 0.1 mmol/kg doses of gadobenate dimeglumine ( Gd-BOPTA ) and gadopentetate dimeglumine ( Gd-DTPA ) for accuracy of detection and characterization of breast lesions on contrast-enhanced MR...
title: Atmosphere circulation patterns synchronize pan-Arctic glacier melt and permafrost thaw
Creators: name: Sasgen, Ingo
name: Steinhoefel, Grit
name: Kasprzyk, Caroline
name: Matthes, Heidrun
name: Westermann, Sebastian
name: Boike, Julia
name: Grosse, Guido
Publisher: name: Humboldt-Universität zu Berlin
Year: 2024
Subjects: subject: Atmospheric dynamics
subject: Climate change
subject: Cryospheric science
subject: 333.7 Landflächen, Naturräume für Freizeit und Erholung, Naturreservate, Energie
subject: 550 Geowissenschaften

description: The Arctic is changing rapidly due to the amplification of global temperature trends, causing profound impacts on the ice sheet in Greenland, glaciers, frozen ground, ecosystems, and societies. Here, we focus on impacts that atmospheric circulation causes in addition to the climate warming trends. We combine time series of glacier mass balance from temporal satellite gravimetry measurements (GRACE/GRACE-FO; 2002–2023), active layer thickness in permafrost areas from ESA’s Climate Change Initiative remote sensing and modelling product (2003–2019), and field measurements of the Circumpolar Active Layer Monitoring Network (2002–2023). Despite regional and system-related complexities, we identify robust covariations between these observations, which vary asynchronously between neighbouring regions and synchronously in regions antipodal to the North Pole. We reveal a close connection with dominant modes of atmosphere circulation, controlling about 75% of the common pan-Arctic impact variability (2002–2022), also affecting the Greenland Ice Sheet. We emphasize that it is necessary to consider such atmospheric driving patterns when projecting impacts, particularly caused by extremes, in an increasingly warmer Arctic.
Nardus stricta 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
Liliopsida
Poales
Poaceae
Nardus
Nardus stricta

description: Nardus stricta Linnaeus, Species Plantarum 1: 53. 1753.
"Habitat in Europae asperis, sterilibus, duris." RCN: 444.
Lectotype (Cope in Jarvis & al., Regnum Veg. 127: 69. 1993): Herb. Linn. No. 73.5 (LINN).
Generitype of Nardus Linnaeus (vide Hitchcock, Prop. Brit. Bot.: 119. 1929).
Current name: Nardus stricta L. (Poaceae).
Note: Although Kerguélen (in Lejeunia, n.s., 75: 215. 1975) indicated unspecified material in LINN as type, this is not accepted as an effective typification (Art. 7.11). See Cafferty & al. (in Taxon 49: 240. 2000) for a detailed explanation.
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 692, DOI: 10.5281/zenodo.291971
GRB Afterglow of the Sub-relativistic Materials with Energy Injection
Creators: name: Fraija, N.
name: Kamenetskaia, B. Betancourt
name: Galvan-Gamez, A.
name: Dainotti, M. G.
name: Becerra, R. L.
name: Dichiara, S.
name: Veres, P.
name: Pedreira, A. C. Caligula do E. S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Sub-relativistic materials launched during the merger of binary compact objects and the core-collapse of massive stars acquire velocity structures when expanding in a stratified environment. The remnant (either a spinning magnetized neutron star (NS) or a central black hole) from the compact-object or core-collapse could additionally inject energy into the afterglow via spin-down luminosity or/and by accreting fall-back material, producing a refreshed shock, modifying the dynamics, and leading to rich radiation signatures at distinct timescales and energy bands with contrasting intensities. We derive the synchrotron light curves evolving in a stratified environment when a power-law velocity distribution parametrizes the energy of the shock, and the remnant continuously injects energy into the blastwave. As the most relevant case, we describe the latest multi-wavelength afterglow observations ($\gtrsim 900$ days) of the GW170817/GRB 170817A event via a synchrotron afterglow model with energy injection of a sub-relativistic material. The features of the remnant and the synchrotron emission of the sub-relativistic material are consistent with a spinning magnetized NS and the faster "blue" kilonova afterglow, respectively. Using the multi-band observations of some short-bursts with evidence of kilonova, we provide constraints on the expected afterglow emission.
description: 36 pages, 14 figures, accepted for publication in ApJ
Sonnenfleckenzeichnung Nr. 71.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 02.04.1969, 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. 28.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 01.02.1969, 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: Genetic structure and effective population size of the European anchovy (Engraulis encrasicolus, L) in the Bay of Biscay
Creators: name: Montes, I.
name: Zarraonaindia, I.
name: Iriondo, M.
name: Grant, W. S.
name: Manzano, C.
name: Abad, D.
name: Carvalho, G. R.
name: Cotano, U.
name: Santos, M.
name: Conklin, D.
name: Irigoien, X.
name: Estonba, A.
Publisher: name: ASC 2015 - Theme session I
Year: 2024
Subjects: Technologies and data
Pressures, impacts, conservation, and management

description: No abstracts are to be cited without prior reference to the author.European anchovy (Engraulis encrasicolus, L) is a small teleost with major socio-economic importance that fuels research efforts. From a conservative perspective, the Bay of Biscay anchovy is especially relevant due to its recent stock collapse, whose biomass began to decline in 2002 and did not recover until 2010, after 5 years without fishing. This slow recovery has raised questions about sustainability of this population, due to the putative loss of adaptive potential, thus leading to final collapse. However, there are few studies about population genetics of this species in the Bay of Biscay. Otolith microchemistry and neutral genetic markers have shown heterogeneity in the anchovy of this region, but mechanisms producing such differences are not fully understood. Here, 456 gene-associated SNPs were analyzed for assessing the fine-scale genetic structure and conservative issues of the Bay of Biscay anchovy. Two major populations with different ecologies associated with different habitats were found in the this region: (1) a large population associated with high-salinity oceanic waters, and (2) a minor inshore population associated with low-salinity estuaries. Individuals from both populations co-mingle during spawning period, therefore, a barrier to gene flow could exist. Regarding conservation, biomass (Nc) fluctuations throughout the stock collapse did not significantly affected genetic diversity (Ne) of the major Bay of Biscay anchovy population. Therefore, this population did not face any severe threat of losing evolutionary potential due to genetic drift and the population recovery during the stock collapse was not impaired by reduced diversity.
‘There’s not a lot of places for them to go’: rural and remote family perspectives on children’s independent mobility
Creators: name: Pelletier, Chelsea
name: Cornish, Katie
name: Sanders, Caroline
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Children’s independent mobility (CIM) is the freedom of children to move around their neighbourhood or community without adult supervision. The aim of this study was to explore experiences with CIM from the perspectives of children and their parents living in rural and remote areas of British Columbia, Canada. Semi-structured interviews were conducted with 21 parent–child dyads or triads (45 participants). Child participants aged 7–12 were invited to create and describe drawings, maps, or take images of their independent mobility. Artwork and interview transcripts were analysed following an inductive thematic approach and mapped to the social-ecological model. We developed four themes to describe rural and remote family perspectives on CIM: (1) natural places, spaces, and forces; (2) embracing informal and unstructured play destinations; (3) decision-making and knowing when they are ready; (4) neighbourhood and community environments. Children identified several environmental characteristics impacting their independent mobility including wildlife, seasonal weather patterns, and lack of destinations. Parents reported the environment of rural communities, including neighbourhood cohesiveness and people looking out for each other, as being supportive of CIM. To promote CIM in rural and remote areas, efforts should focus on providing education on wildlife encounters, creating safe and interesting destinations for play, and consider children’s safety and connectivity in road design.
Sonnenfleckenzeichnung Nr. 62.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 24.03.1969, 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
Sonnenfleckenzeichnung Nr. 112.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.05.1969, 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
title: MR guided breast biopsy in high risk women for breast cancer: Results and recommendations
Creators: name: Ferré, Romuald
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: PROBLEMATICS: Breast MRI has a 86-100% rate of sensitivity and a variable specificity rate (20-100%) for the detection of breast cancer When suspicious breast lesions are detected at MRI, they need to be characterized by a biopsy In 50% of cases,...
FEATURES OF ABDOMІNOPLASTY MODELING IN THE EXPERIMENT
Creators: name: Trombola O., V.
Publisher: name: Zenodo
Year: 2022

description: Абдомінопластика є однією з найпопулярніших операцій в пластичній хірургії. Незважаючи на низький рівень післяопераційних ускладнень, що за міжнародними дослідженнями складає 4%, в їх число, окрім гематом та інфекцій, входить і венозний тромбоемболізм, що може спричинити летальні наслідки. Для їх профілактики важливо розуміти патоморфологічні зміни тканин передньої черевної стінки після проведення абдомінопластики. Оскільки дані дослідження передбачають значні труднощі, розробка експериментальної моделі абдомінопластики є актуальною.
Synthesis and Properties of Non-Curing Graphene Thermal Interface Materials
Creators: name: Naghibi, Sahar
name: Kargar, Fariborz
name: Wright, Dylan
name: Huang, Chun Yu Tammy
name: Mohammadzadeh, Amirmahdi
name: Barani, Zahra
name: Salgado, Ruben
name: Balandin, Alexander
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Development of the next generation thermal interface materials with high thermal conductivity is important for thermal management and packaging of electronic devices. We report on the synthesis and thermal conductivity measurements of non-curing thermal paste, i.e. grease, based on mineral oil with the mixture of graphene and few-layer graphene flakes as the fillers. It was found that graphene thermal paste exhibits a distinctive thermal percolation threshold with the thermal conductivity revealing a sublinear dependence on the filler loading. This behavior contrasts with the thermal conductivity of curing graphene thermal interface materials, based on epoxy, where super-linear dependence on the filler loading is observed. The performance of graphene thermal paste was benchmarked against top-of-the-line commercial thermal pastes. The obtained results show that non-curing graphene thermal interface materials outperforms the best commercial pastes in terms of thermal conductivity, at substantially lower filler concentration of ~ 27 vol%. The obtained results shed light on thermal percolation mechanism in non-curing polymeric matrices laden with quasi-two-dimensional fillers. Considering recent progress in graphene production via liquid phase exfoliation and oxide reduction, we argue that our results open a pathway for large-scale industrial application of graphene in thermal management of electronics.
description: 29 pages, 7 figures
Nauclea orientalis Linnaeus 1762
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
Gentianales
Rubiaceae
Nauclea
Nauclea orientalis

description: Nauclea orientalis (Linnaeus) Linnaeus, Species Plantarum, ed. 2, 1: 243. 1762.
"Habitat in India Asiatica." RCN: 1350.
Basionym: Cephalanthus orientalis L. (1753).
Lectotype (Merrill in J. Washington Acad. Sci. 5: 533. 1915): Herb. Hermann 5: 338, No. 53 [icon] (BM-000621104).
Generitype of Nauclea Linnaeus.
Current name: Nauclea orientalis (L.) L. (Rubiaceae).
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 692, DOI: 10.5281/zenodo.291971
title: Correlation of enhancement in breast MRI with histologic markers
Creators: name: Diekmann, Felix
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 the present study was to histologically determine the capillary density of breast lesions using histologic markers D2-40, CD31, and CD34 and to correlate the results with early contrast enhancement in magnetic resonance (MR) mammography...
Sonnenfleckenzeichnung Nr. 229.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 20.09.1969, 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
Neutrino pair annihilation above black-hole accretion disks in modified gravity
Creators: name: Lambiase, G.
name: Mastrototaro, L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Using idealized models of the accretion disk, we investigate the effects induced by the modified theories of gravity on the annihilation of the neutrino pair annihilation into electron-positron pairs ($ν{\bar ν}\to e^-e^+$), occurring near the rotational axis. For the accretion disk, we have considered the models with temperature $T=constant$ and $T\propto r^{-1}$. In both cases, we find that the modified theories of gravity lead to an enhancement, up to more than one order of magnitude with respect to General Relativity, of the rate of the energy deposition rate of neutrino pair annihilation.
description: 12 pages, 4 figure. Accepted for publication on ApJ
Type III Neutrino Seesaw, Freeze-In Long-Lived Dark Matter, and the $W$ Mass Shift
Creators: name: Ma, Ernest
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the framework of seesaw neutrino masses from heavy fermion triplets $(Σ^+,Σ^0,Σ^-)$, the addition of a light fermion singlet $N$ and a heavy scalar triplet $(ρ^+,ρ^0,ρ^-)$ has some important consequences. The new particles are assumed to be odd under a new $Z_2$ symmetry which is only broken softly, both explicitly and spontaneously. With $N-Σ^0$ mixing, freeze-in long-lived dark matter through Higgs decay becomes possible. At the same time, the $W$ mass is shifted slightly upward, as suggested by a recent precision measurement.
description: 6 pages, 2 figures, typos corrected
On the existence of Auslander-Reiten (d+2)-angles in (d+2)-angulated categories
Creators: name: Zhou, Panyue
Publisher: name: arXiv
Year: 2019
Subjects: subject: Representation Theory (math.RT)
subject: Category Theory (math.CT)
subject: FOS: Mathematics
subject: 16G70, 18E30

description: Let $\cal C$ be a $(d+2)$-angulated category. In this note, we show that if $\cal C$ is a locally finite, then $\cal C$ has Auslander-Reiten $(d+2)$-angles. This extends a result of Xiao-Zhu for triangulated categories.
description: 16 pages. arXiv admin note: text overlap with arXiv:1910.01454
Nepenthes distillatoria Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Caryophyllales
Nepenthaceae
Nepenthes
Nepenthes distillatoria

description: Nepenthes distillatoria Linnaeus, Species Plantarum 2: 955. 1753.
"Habitat in Zeylona." RCN: 6913.
Lectotype (designated here by Cheek): Herb. Hermann 3: 52, No. 321 (BM).
Generitype of Nepenthes Linnaeus.
Current name: Nepenthes distillatoria L. (Nepenthaceae).
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 692, DOI: 10.5281/zenodo.291971
Sonnenfleckenzeichnung Nr. 247.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 09.10.1969, 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
Nepeta cataria 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
Lamiaceae
Nepeta
Nepeta cataria

description: Nepeta cataria Linnaeus, Species Plantarum 2: 570. 1753.
"Habitat in Europa." RCN: 4168.
Lectotype (Ubera & Valdés in Lagascalia 12: 17. 1983): Herb. Linn. No. 726.1 (LINN).
Generitype of Nepeta Linnaeus (vide Green, Prop. Brit. Bot.: 164. 1929).
Current name: Nepeta cataria L. (Lamiaceae).
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 692, DOI: 10.5281/zenodo.291971
Deformed Infinite series metric in Cartan Spaces
Creators: name: Tripathi, Brijesh Kumar
name: Chaubey, V. K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C60, 53B40

description: Igarashi introduce the concept of $(α, β)$-metric in Cartan space $\ell^{n}$ analogously to one in Finsler space and obtained the basic important geometric properties and also investigate the special class of the space with $(α, β)$-metric in $\ell^{n}$ in terms of $ 'invariants' $. In the present paper we determine the $ 'invariants' $ in two different cases of deformed infinite series metric which characterize the special classes of Cartan spaces $\ell^{n}$.
Possible detection of coronal mass ejections on late-type main-sequence stars in LAMOST medium-resolution spectra
Creators: name: Lu, Hong-peng
name: Tian, Hui
name: Zhang, Li-yun
name: Karoff, Christoffer
name: Chen, He-chao
name: Shi, Jian-rong
name: Hou, Zhen-yong
name: Chen, Ya-jie
name: Xu, Yu
name: Wu, Yu-chuan
name: Cao, Dong-tao
name: Wang, Jiang-tao
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Stellar coronal mass ejections (CMEs) are the primary driver of the exoplanetary space weather and they could affect the habitability of exoplanets. However, detections of possible stellar CME signatures are extremely rare. Aims. This work aims to detect stellar CMEs from time-domain spectra observed through the LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS). Our sample includes 1,379,408 LAMOST-MRS spectra of 226,194 late-type main-sequence stars ($\rm T_{eff} < 6000$ K, $\rm log [g/(cm\ s^{-2})] > 4.0$). Methods. We first identified stellar CME candidates by examining the asymmetries of H$α$ line profiles, and then performed double Gaussian fitting for H$α$ contrast profiles (differences between the CME spectra and reference spectra) of the CME candidates to analyze the temporal variation of the asymmetric components. Results. Three stellar CME candidates were detected on three M dwarfs. The H$α$ and Mg I triplet lines (at 5168.94 Å, 5174.13 Å, 5185.10 Å) of candidate 1 all exhibit a blue-wing enhancement, and the corresponding Doppler shift of this enhancement shows a gradually increasing trend. The H$α$ line also shows an obvious blue-wing enhancement in candidate 2. In candidate 3, the H$α$ line shows an obvious red-wing enhancement, and the corresponding projected maximum velocity exceeds the surface escape velocity of the host star. The lower limit of the CME mass was estimated to be $\sim$$8 \times 10^{17}$ g to $4 \times 10^{18}$ g for these three candidates.
description: Accepted by A&A
title: Contrast-enhanced magnetic resonance imaging as problem solving tool in BIRADS 3 breast lesions
Creators: name: Dorrius, Monique
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: According to the guideline ofAHRQ (1) and NABON (2) the work-up of mammographic BIRADS 3 lesion should be: –a biopsy or –follow-up after 6 months The additional value of breast contrast-enhanced Magnetic Resonance Imaging (MRI) in BIRADS 3...
Sonnenfleckenzeichnung Nr. 192.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 12.08.1969, 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
The one-loop amplitudes for Higgs + 4 partons with full mass effects
Creators: name: Budge, Lucy
name: Campbell, John M.
name: De Laurentis, Giuseppe
name: Ellis, R. Keith
name: Seth, Satyajit
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present compact analytic formulae for the one-loop amplitudes for Higgs + 4 parton scattering, $0 \to g g g g h$, $0 \to \bar{q} q gg h$ and $0\to \bar{q} q \bar{q}^\prime q^\prime h$, mediated by a loop of massive coloured quarks. We exploit the correspondence with a theory in which a massive coloured scalar circulates in the loop to avoid a proliferation in the number of terms in the result. In addition, we use momentum twistors and high precision numerical evaluations to simplify the expressions. The analytic results in this paper, in terms of spinor products, allow construction of an efficient numerical program to calculate the amplitude.
description: 45 pages, 1 figure; v3 updated to published version, corrected typo in Eq. (5.1), added missing reference
Sonnenfleckenzeichnung Nr. 3.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 03.01.1969, 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