cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Wrightia antidysenterica R. Br.
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
Apocynaceae
Wrightia
Wrightia antidysenterica

description: Nerium antidysentericum Linnaeus, Species Plantarum 1: 209. 1753.
"Habitat in India." RCN: 1717.
Lectotype (Trimen, Handb. Fl. Ceylon 3: 138. 1895): Herb. Hermann 4: 76, No. 107 (BM-000594775).
Current name: Wrightia antidysenterica (L.) R. Br. (Apocynaceae).
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 693, DOI: 10.5281/zenodo.291971
title: Joined-Up Thinking from Joined -UP Data
Creators: name: Currie, David
name: Gault, Jeremy
name: Kelly, Ciaran
Publisher: name: ASC 2015 - Theme session L
Year: 2024
Subjects: The sea and human culture and societies
Ecosystem observation, processes and dynamics

description: No abstracts are to be cited without prior reference to the author.Fisheries data is not managed in a vacuum and the data management issues often encountered are not solely technical but include an administrative dimension. Ireland, in common with many other EU member states, has a number of bodies responsible for the different types of data utilised for scientific and fisheries reporting purposes. We have successfully mapped out the fishery data management landscape in Ireland and how data is produced, exchanged, and utilised. In particular we compared and contrasted the technical problems and their resolutions with the legal, policy, and procedural issues in order to illuminate how practical solutions must be designed.
Gardenia jasminoides J. Ellis 1761
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
Gardenia
Gardenia jasminoides

description: Nerium floridum Linnaeus, Mantissa Plantarum Altera: 346. 1771, nom. illeg.
["Habitat in India orientali: Suratte, Amboina, Cap. b. spei."] Sp. Pl., ed. 2, 1: 305 (1762). RCN: 1709.
Replaced synonym: Gardenia jasminoides J. Ellis (1761); G. florida L. (1762), nom. illeg.
Type not designated.
Current name: Gardenia jasminoides J. Ellis (Rubiaceae).
Note: A recombination of Gardenia florida L. (1762), itself an illegitimate renaming of G. jasminoides J. Ellis (1761).
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 693, DOI: 10.5281/zenodo.291971
title: Implementation of diffusion weighted imaging into an MR-enterography protocol: A feasibility study
Creators: name: Paolantonio, Pasquale
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 assess the feasibility of diffusion weighted imaging (DWI) of the small bowel and to identify the appearance of inflammatory changes of the small bowel wall in Crohn’s at...
PRINCIPLES OF BIOETHICS IN TREATMENT AND REHABILITATION OF PATIENTS WITH СHRONIC KIDNEY DISEASE
Creators: name: LD, Denova
Publisher: name: Zenodo
Year: 2022

description: The modern concept of "bioethics" is closely intertwined with the concepts of "deontology", "doctor's code of ethics". From the moment of conception until the death of the patient, the doctor's activities should be aimed at preserving the life and health of the patient and requires him to treat the patient humanely as a person, respect his personality, show compassion and complicity, benevolence, charity and mercy, patience, mutual trust, decency, and justice. Conscience must be the chief judge in his professional path. These moral principles are systematized in the Code of Ethics of Physicians of Ukraine (hereinafter - the Code) taking into account the provisions of the International Code of Ethics, the Helsinki Declaration, the Universal Declaration on Genome and Human Rights and the Convention for the Protection of Human Rights and Dignity. This Code was created for use in the professional activities of physicians and scientists whose professional activities cover prenatal and postnatal life and human health, birth, and death.
Sonnenfleckenzeichnung Nr. 301.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 13.12.1969, 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. 19.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 22.01.1969, 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
A model for the possible connection between tidal disruption event and quasi-periodic eruption in GSN 069
Creators: name: Wang, Mengye
name: Yin, Jinjing
name: Ma, Yiqiu
name: Wu, Qingwen
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Quasi-periodic eruptions (QPEs) are found in the center of five galaxies, where a tidal disruption event (TDE)-like event is also reported in GSN 069 that happened a couple of years before the QPEs. We explain the connection of these phenomena based on a model of a highly eccentric white-dwarf (WD)-$10^{4-6}M_{\odot}$ massive black hole (MBH) binary formed by the Hill mechanism. In this system, the tidal induced internal oscillation of WD can heat the WD envelope thereby induces the tidal nova and inflates the WD envelope, which can be captured by the MBH and form a TDE. The tidal stripping of the surviving WD in the eccentric orbit can produce the QPEs. We also apply this model to the other four QPE sources. Based on the estimated fallback rate, we find that the remaining time after the QPE-observed time for these QPEs is only around 1-2 years based on our simple model estimation, and then the WD will be fully disrupted. We also show that the accretion rate can be much higher than Eddington accretion rate in final stage of these QPE sources. The peak frequency of spectral energy distribution of disk stays in soft X-ray band ($\sim 0.1-1$ keV), which is consistent with observational results.
description: 12 pages, 8 figures, accepted by ApJ
Sonnenfleckenzeichnung Nr. 281.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.11.1969, 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
Constraining Dark Matter Microphysics with the Annihilation Signal from Subhalos
Creators: name: Runburg, Jack
name: Baxter, Eric J.
name: Kumar, Jason
Publisher: name: arXiv
Year: 2021
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the cold dark matter scenario, galactic dark matter halos are populated with a large number of smaller subhalos. Previous work has shown that dark matter annihilations in subhalos can generate a distinctive, non-Poisson signal in the gamma-ray photon counts probability distribution function (PDF). Here we show that the gamma-ray PDF also carries information about the velocity dependence of the dark matter annihilation cross section. After calculating the PDF assuming $s$-wave and Sommerfeld-enhanced annihilation, we perform a mock data analysis to illustrate how current and future observations can constrain the microphysics of the dark matter annihilation. We find that, with current Fermi data, and assuming a dark matter annihilation cross section roughly at the limit of current bounds from annihilation in dwarf spheroidal galaxies, one can potentially distinguish the non-Poissonian fluctuations expected from dark matter annihilation in subhalos from Poisson sources, as well as from dark matter models with an incorrect velocity-dependence. We explore how robust these results are to assumptions about the modeling of astrophysical backgrounds. We also point out a four-parameter degeneracy between the velocity dependence of the dark matter annihilation, the minimum subhalo mass, the power law index of the subhalo mass function, and the normalization of the dark matter signal. This degeneracy can be broken with priors from N-body simulations or from observational constraints on the subhalo mass function.
description: 26 pages, 7 figures
title: Role of 64-slices MDCT-enterography in the evaluation of patients with suspected small bowel neoplasm
Creators: name: Lo Re, Giuseppe
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 reliability and diagnostic potential of MDCT-Enterography (MDCT-E), an emerging technique of small bowel examination that combines the advantages of MDCT examination of the abdomen and the enteral volume challenge of enterography, in...
title: Gastric banding: What radiologists need to know
Creators: name: Thomas, Davis
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Stomach (incl. Oesophagus)
subject: GI Tract - Stomach

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: Brief review of therelevantfeatures of laparoscopic gastric band surgery,the role of a radiologist and the imaging features thatone might...
title: Knowing the past to improve the future: Estimating historical fishing catches to improve fisheries management in the western Mediterranean Sea.
Creators: name: Carreras, Marta
Publisher: name: ASC 2015 - Theme session L
Year: 2024
Subjects: The sea and human culture and societies
Ecosystem observation, processes and dynamics

description: No abstracts are to be cited without prior reference to the author.We developed for the first time the commercial fishing catches reconstruction of the Balearic Islands(Western Mediterranean) between 1950 and 2010, by adding non‐reported components, includingunreported landings and discards, to the official reported landing data. To back‐estimate historicalunreported landings and discards, collaboration and information acquired from fishermen wereessential, as gathered through interviews and observer programs of the Spanish OceanographicInstitute (IEO) on board commercial bottom trawling fleet. We estimated a total catch of 511,500 t overthe period 1950‐2010, of which official landings represented 49% (around 248,000 t), followed byunreported catches (32%) and discards (20%). A decrease in unreported catches was observed duringthe period 1950‐2010 (from 58% to 38%) due to a reduction of unreported landings, but substantialefforts are still required to improve the recordings of actual fishing catches. This work contributes tothe global assessment of fisheries removals led by the Sea Around Us and aims to provide the basis foran improved management of the Balearic Islands and Mediterranean Sea fisheries.
Sonnenfleckenzeichnung Nr. 69.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 31.03.1969, 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: Preoperative vascular mapping for endoscopic treatment of gastric mucosal neoplasm: New vascular imaging of CT gastrography-wall carving image using MDCT
Creators: name: Tsurumaru, Daisuke
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Stomach (incl. Oesophagus)
subject: GI Tract - Stomach

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Introduction Endoscopic mucosal resection (EMR) and submucosal dissection (ESD) have been accepted as standard treatment strategies for selected cases of early gastric cancer (EGC) 1-3 . Bleeding is the most common complication, with the reported...
Physics of nova outbursts: A theoretical model of classical nova outbursts with self-consistent wind mass loss
Creators: name: Kato, Mariko
name: Saio, Hideyuki
name: Hachisu, Izumi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a model for one cycle of a classical nova outburst based on a self-consistent wind mass loss accelerated by the gradient of radiation pressure, i.e., the so-called optically thick winds. Evolution models are calculated by a Henyey code for a 1.0 $M_\odot$ white dwarf (WD) with a mass accretion rate of $5 \times 10^{-9}~M_\odot$ yr$^{-1}$. The outermost part of hydrogen-rich envelope is connected to a steadily moving envelope when optically thick winds occur. We confirm that no internal shock waves occur at the thermonuclear runaway. The wind mass loss rate reaches a peak of $1.4 \times 10^{-4}~M_\odot$ yr$^{-1}$ at the epoch of the maximum photospheric expansion, where the photospheric temperature decreases to $\log T_{\rm ph}$ (K)=3.90. Almost all of the accreted mass is lost in the wind. The nuclear energy generated in hydrogen burning is lost in a form of photon emission (64 %), gravitational energy (lifting-up the wind matter against the gravity, 35 %), and kinetic energy of the wind (0.23 %). A classical nova should be very bright in a far-UV (100 - 300 Å) band, during a day just after the onset of thermonuclear runaway ($\sim$25 d before the optical maximum). In the decay phase of the nova outburst, the envelope structure is very close to that of a steady state solution.
description: 18 pages including 17 figures, PASJ in press, Fig.10 replaced, typos corrected
title: Gastric band procedure for the treatment of obesity: Imaging findings and protocol
Creators: name: Alves, Nuno
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Gastrointestinal tract
subject: Stomach (incl. Oesophagus)
subject: GI Tract - Stomach

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To illustrate the spectrum of imaging findings resultant of gastric lap-banding, both the normal and complicated. To discuss the best imaging methods to study these situations along with its advantages and...
Multi-wavelength Variation Phenomena of PKS 0735+178 on Diverse Timescale
Creators: name: Fang, Yue
name: Chen, Qihang
name: Zhang, Yan
name: Wu, Jianghua
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: BL Lac object PKS 0735+178 showed some complex multi-wavelength variation phenomena in the previous studies, especially for its color behavior. Bluer-when-brighter, redder-when-brighter and achromatic behavior were all found to be possible long-term trends of PKS 0735+178. In this work, we collected the long-term multi-wavelength data of PKS 0735+178, and also performed a multi-color optical monitoring on intraday timescale. The intraday variability was detected on one night. On the long timescale, a possible 22-day time lag was found between the $R$ and $γ$-ray bands. The results of the cross-correlation analysis exhibited strong correlations between various optical bands on both intraday and long timescale. However, only a mild correlation was found between the long-term $γ$-ray and $R$-band light curves, which could be interpreted by the different emission mechanisms of the $γ$-ray and optical emissions. PKS 0735+178 showed a significant harder-when-brighter in the $γ$-ray band, which is consistent with the observed optical bluer-when-brighter trend on both long-term and intraday timescales. We found that the HWB and BWB trends will be enhanced during the active states, especially for the historical low state. Such phenomenon indicates a special activity-dependent color behavior of PKS 0735+178, and it could be well interpreted by the jet emission model.
description: Accepted for publication in ApJ, 19 pages, 13 figures
ЗАСАДИ ФІЛОСОФСЬКОЇ АНТРОПОЛОГІЇ
Creators: name: Буцикін, Єгор
Publisher: name: Zenodo
Year: 2022

description: Цього року маємо 95 річницю оприлюднення тексту «Становище людини в космосі», що він започаткував традицію європейської філософської антропології, чи ліпше сказати, нової філософської антропології саме як методологічної настанови. Варто заказати, що філософську антропологію можна розуміти подвійно, з одного боку як дисципліну історії філософії, що має за об’єкт розмаїті вчення про природу й сутність людини, з другого – як осібну методологічну настанову, яка має на меті обґрунтування предметної царини природничих і гуманітарних наук і утворення не одностороннього, а сутнісного поняття людини. Мені передусім ідеться про антропологію у другому сенсі. Сучасна філософська антропологія не є методологічно однорідною, а радше пов’язана спільною зацікавленістю до предмету – «людина» і підходом, що його влучно назвав Ото Больнов «антропологічною редукцією». Цей підхід полягає у зведенні усього багатоманіття переживань людини до екзистенційної фактичності людського існування чи, інакше кажучи, антропологічної ситуації. Ця фактичність постає як випадковість, що має універсальний і смислоконститутивний стосунок до людського досвіду, а також саморозуміння.
Explicit construction of $N = 2$ SCFT orbifold models. Spectral flow and mutual locality
Creators: name: Belavin, Alexander
name: Belavin, Vladimir
name: Parkhomenko, Sergey
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work we present a new approach to constructing Calabi-Yau orbifold models required for compactification in superstring theory. We use the connection of CY orbifolds with the class of exactly solvable N=2 SCFT models to explicitly construct a complete set of fields in these models using the twisting of the spectral flow and the requirement of mutual locality of the fields.
description: References added, minor corrections
Nerium oleander 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
Gentianales
Apocynaceae
Nerium
Nerium oleander

description: Nerium oleander Linnaeus, Species Plantarum 1: 209. 1753.
"Habitat in Creta, Palaestina, Syria, India." RCN: 1715.
Lectotype (Stearn in Davis, Fl. Turkey 6: 159. 1978): Herb. Clifford: 76, Nerium 1 β (BM-000558145).
Generitype of Nerium Linnaeus (vide Steudel, Nom. 1: 553. 1821).
Current name: Nerium oleander L. (Apocynaceae).
Note: Pagen (in Agric. Univ. Wageningen Pap. 87-2: 7. 1987) illustrates the lectotype, as well as (pp. 44-48) illustrations from Dodoëns, Hermann, Rheede and Weinmann.
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 693, DOI: 10.5281/zenodo.291971
title: Carcinosarcoma/Metaplastic carcinoma of the breast: multi-institutional study with clinical, pathologic and imaging features in 47 patients
Creators: name: Utrilla, Cristina
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: Oncology
subject: Neoplasia
subject: Breast - Tumors

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To review clinical and pathological features of carcinosarcoma/metaplastic carcinoma of the breast(CS/MCB) in a large serie of patients in two institutions To show imaging findings and to correlate them with histopahologic...
The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines
Creators: name: Markov, Vladan
name: Carniani, Stefano
name: Vallini, Livia
name: Ferrara, Andrea
name: Pallottini, Andrea
name: Maiolino, Roberto
name: Gallerani, Simona
name: Pentericci, Laura
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A tight relation between [C II] line luminosity and the star formation rate (SFR) has been observed for local galaxies. At high redshift (z > 5), galaxies instead deviate downwards from the local $Σ$_[C II] - $Σ$_SFR relation. This deviation might be caused by different interstellar medium (ISM) properties in galaxies at early epochs. To test this hypothesis, we combined the [C II] and SFR data with C III] line observations and our physical models. We additionally investigated how ISM properties, such as burstiness, $κ_s$, total gas density, $n$, and metallicity, $Z$, affect the deviation from the $Σ$_[C II] - $Σ$_SFR relation in these sources. We present the VLT/X-SHOOTER observations targeting the C III] $λ1909$ line emission in three galaxies at 5.5 < z < 7. We include X-SHOOTER and VLT/MUSE archival data of eight galaxies at 2 < z < 7, and eleven star-forming systems at 6 < z < 7.5, with either C III] or [C II] detection reported in the literature. We detected C III] $λλ1907, 1909$ line emission in HZ10 and we derived the intrinsic, integrated flux of the C III] $λ1909$ line. We constrained the ISM properties for our sample of galaxies, $κ_s$ , $n$, and $Z$, by applying our physically motivated model based on the MCMC algorithm. For the most part, high-z star-forming galaxies show subsolar metallicities. The majority of the sources have $log(κ_s) > 1$, that is, they overshoot the Kennicutt-Schmidt (KS) relation by about one order of magnitude, implying that the whole KS relation might be shifted upwards at early times. Furthermore, all the high-z galaxies of our sample lie below the $Σ$_[C II] - $Σ$_SFR local relation. The total gas density, $n$, shows the strongest correlation with the deviation from the local $Σ$_[C II] - $Σ$_SFR relation.
description: 16 pages, 13 figures, to be published in A&A
Sonnenfleckenzeichnung Nr. 253.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.10.1969, 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
Energy-Based Generative Cooperative Saliency Prediction
Creators: name: Zhang, Jing
name: Xie, Jianwen
name: Zheng, Zilong
name: Barnes, Nick
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Conventional saliency prediction models typically learn a deterministic mapping from an image to its saliency map, and thus fail to explain the subjective nature of human attention. In this paper, to model the uncertainty of visual saliency, we study the saliency prediction problem from the perspective of generative models by learning a conditional probability distribution over the saliency map given an input image, and treating the saliency prediction as a sampling process from the learned distribution. Specifically, we propose a generative cooperative saliency prediction framework, where a conditional latent variable model (LVM) and a conditional energy-based model (EBM) are jointly trained to predict salient objects in a cooperative manner. The LVM serves as a fast but coarse predictor to efficiently produce an initial saliency map, which is then refined by the iterative Langevin revision of the EBM that serves as a slow but fine predictor. Such a coarse-to-fine cooperative saliency prediction strategy offers the best of both worlds. Moreover, we propose a "cooperative learning while recovering" strategy and apply it to weakly supervised saliency prediction, where saliency annotations of training images are partially observed. Lastly, we find that the learned energy function in the EBM can serve as a refinement module that can refine the results of other pre-trained saliency prediction models. Experimental results show that our model can produce a set of diverse and plausible saliency maps of an image, and obtain state-of-the-art performance in both fully supervised and weakly supervised saliency prediction tasks.
title: Carcinoma of the breast and meningioma: Associated tumors or random events?
Creators: name: Georgiou, Irene
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: Oncology
subject: Neoplasia
subject: Breast - Tumors

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To illustrate the association between breast cancer and meningioma that indicates a possible epidemiologic, hormonal and genetic...
title: Pulse trawling as an alternative for beam trawling: insights from a spatial-agent based model
Creators: name: Sys, Klaas
name: van Meensel, Jef
name: Buysse, Jeroen
name: Polet, Hans
Publisher: name: ASC 2015 - Theme session M
Year: 2024
Subjects: The sea and human culture and societies
Ecosystem observation, processes and dynamics

description: No abstracts are to be cited without prior reference to the author.Changed socio-economic, ecological and institutional conditions increased the pressure on the beam trawler fishery using tickler chains. Pulse trawling, in which the tickler chains are replaced by electrodes, is seen as an alternative for the beam trawler fleet targeting sole (Solea solea). In this study, a spatial agent-based fleet dynamic model is developed to gain more insights in the socio-economic and ecological effects of the introduction of four pulse trawlers in the Belgian beam trawler fleet (>221 kW). This fleet practices different métiers whereby other fish species than sole have an important value in the total landed revenue. In the scenario without landing obligation, pulse trawlers have mainly ecological advantages. Fuel usage is lower and the discards of marketable plaice and undersized species are lower, however the difference in profitability is less pronounced due to lower landings of other target species. With landing obligation, pulse trawling is more profitable because the quota for the choke species are not as soon depleted as for beam trawlers. As such pulse trawlers are able to spend more days at sea.
title: Unfrequent manifestations of breast tumors on mammography and ultrasound
Creators: name: Broncano Cabrero, Jordi
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: Oncology
subject: Neoplasia
subject: Breast - Tumors

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To show some rare and atypical mammographic and ultrasonographic manifestations of breast cancer,such as: malignant microcalcifications located in the skin, carcinoma in ectopic axillary tissue, multifocal mucinous carcinoma showing as ductal...
title: Invasive pleomorphic lobular carcinoma and classic invasive lobular carcinoma: What’s the difference?
Creators: name: Seco, Miguel
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: Oncology
subject: Neoplasia
subject: Breast - Tumors

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: This study aims to characterize a series of pleomorphic lobular carcinoma (PLC) from the clinical, radiological histological and imunohistochemical characteristics. In addition, these aspects are compared with invasive lobular carcinoma (ILC) of...
Models of Millimeter and Radio Emission from Interacting Supernovae
Creators: name: Yadlapalli, Nitika
name: Ravi, Vikram
name: Ho, Anna Y. Q.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: This work utilizes established models of synchrotron-powered light curves for core-collapse supernovae in dense circumstellar environments, namely type IIn and Ibn, to demonstrate the potential for detecting millimeter emission from these events. The progenitor types of these supernovae are still an open question, but using the synchrotron light curves as probes for the circumstellar environments could shed light on the mass-loss histories of the progenitors and discern between different theories. Observations in millimeter bands are particularly fruitful, as they probe regions at smaller radii and higher ambient densities, where centimeter emission tends to be self-absorbed. In our application of these light curves, we explore a diversity of progenitor types and mass-loss profiles to understand their effects on the light curve shapes. Additionally, we fit model parameters to the 8\,GHz light curve of type IIn supernova 2006jd and then create millimeter light curves using these parameters to show the possibility of detecting an early millimeter peak from such an event. We predict that next generation millimeter surveys will possess the capability to detect nearby and extreme events. However, there is a pressing need for millimeter follow-up of optically discovered interacting supernovae to more completely sample the true population.
description: 12 pages, 6 figures, accepted for publication in ApJ
Sonnenfleckenzeichnung Nr. 18.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.01.1969, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
title: Breast tumor in young diabetic patients: A diagnostic challenge
Creators: name: Medina, Rosana
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Breast
subject: Oncology
subject: Neoplasia
subject: Breast - Tumors

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: BACKGROUND AND PURPOSE. Diabetic fibrous mastopathy is a rare entity that mimics breast carcinoma.This disease was first described in 1984 by Soler and Khardori in premenopausal woman with insulin-dependent diabetes. [1].The majority of these...
Sonnenfleckenzeichnung Nr. 303.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.12.1969, 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: Risk factors in implementation of speech recognition system into daily use of radiologists
Creators: name: Ahovuo, Juhani
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: Speech recognition (SR) has become a tool in reporting of the results of medical imaging examinations. Eveyone planning to implement a SR system into the daily use shall notice that this is a change process and it needs appropriate management. This...
Multireference configuration interaction study of the predissociation of C$_{2}$ via its $F\,^1Π_u$ state
Creators: name: Xu, Zhongxing
name: Federman, S. R.
name: Jackson, William M.
name: Ng, Cheuk-Yiu
name: Wang, Lee-Ping
name: Crabtree, Kyle N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Photodissociation is one of the main destruction pathways for dicarbon (C$_{2}$) in astronomical environments such as diffuse interstellar clouds, yet the accuracy of modern astrochemical models is limited by a lack of accurate photodissociation cross sections in the vacuum ultraviolet range. C$_{2}$ features a strong predissociative $F\,^1Π_u - X\,^1Σ_g^+$ electronic transition near 130 nm originally measured in 1969; however, no experimental studies of this transition have been carried out since, and theoretical studies of the $F\,^1Π_u$ state are limited. In this work, potential energy curves of excited electronic states of C$_{2}$ are calculated with the aim of describing the predissociative nature of the $F\,^1Π_u$ state and providing new ab initio photodissociation cross sections for astrochemical applications. Accurate electronic calculations of 56 singlet, triplet, and quintet states are carried out at the DW-SA-CASSCF/MRCI+Q level of theory with a CAS(8,12) active space and the aug-cc-pV5Z basis set augmented with additional diffuse functions. Photodissociation cross sections arising from the vibronic ground state to the $F\,^1Π_u$ state are calculated by a coupled-channel model. The total integrated cross section through the $F\,^1Π_u$ $v=0$ and $v=1$ bands is 1.198$\times$10$^{-13} $cm$^2$cm$^{-1}$, giving rise to a photodissociation rate of 5.02$\times$10$^{-10}$ s$^{-1}$ under the standard interstellar radiation field, much larger than the rate in the Leiden photodissociation database. In addition, we report a new $2\,^1Σ_u^+$ state that should be detectable via a strong $2\,^1Σ_u^+-X\,^1Σ_g^+$ band around 116 nm.
description: 33 pages, 13 figures; Accepted by The Journal of Chemical Physics
title: Teleradiological evaluation of MDCT examinations of skull injuries: 2D or 3D images first?
Creators: name: Gmur, Aleksander
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: To present value of 3D volume rendered images of the skull in case of head trauma patients with the use of MDCT and teleradiology. To choose which type of images (2D or 3D) should be viewed at the beginning of study...
Sonnenfleckenzeichnung Nr. 68.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 30.03.1969, 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
Limits on the Auroral Generation of H$_3^+$ in Brown Dwarf and Extrasolar Giant Planet Atmospheres with Keck/NIRSPEC
Creators: name: Gibbs, Aidan
name: Fitzgerald, Michael
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The molecular ion H$_3^+$ is a potentially powerful tracer of the ionospheres and thermal structures of Jovian planets, but has never been detected in a planetary mass object outside of the solar system. Models predict that H$_3^+$ emission driven by EUV flux and solar wind on hot Jupiters, or by powerful aurorae on brown dwarfs, will be between $10^2$ and $10^5\times$ more intense than that of Jupiter. If optimal conditions for the production of emission do exist, the emission may be detectable by current ground-based instruments or in the near future. We present the first search for H$_3^+$ line emission in brown dwarfs with Keck/NIRSPEC $L^\prime$ high-resolution spectroscopy. Additionally, we survey stars hosting giant planets at semi-major axes near $0.1-0.2$ au, which models suggest may be the best planetary targets. No candidate H$_3^+$ emission is found. The limits we place on the emission of H$_3^+$ from brown dwarfs indicates that auroral generation of H$_3^+$ in these environments likely does not linearly scale from the processes found on Jupiter, plausibly due to deeper atmospheric penetration by precipitating auroral electrons. Detection of H$_3^+$ emission in brown dwarfs may be possible with the James Webb Space Telescope (JWST), or future thirty-meter class telescopes.
description: 22 pages, 12 figures
Sonnenfleckenzeichnung Nr. 259.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.10.1969, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1969

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert
title: Easy, fast and accurate: Manual segmentation of CT scans for precise volumetry and surface reconstruction on tablet monitor
Creators: name: Simon, Martin
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Learning objectives Background Imaging findings OR Procedure details Conclusion Personal Information References
description: Learning objectives: In modern human medicine the volumetry of organs and structures gains more and more importance for follow-up therapy. Therefore, easy, fast and accurate methods of CT-scan segmentation and the definition of corresponding normal values are...
Sonnenfleckenzeichnung Nr. 289.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.11.1969, 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
Wrightia antidysenterica R. Br.
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
Apocynaceae
Wrightia
Wrightia antidysenterica

description: Nerium zeylonicum Linnaeus, Centuria II Plantarum: 12. 1756.
"Habitat in India." RCN: 1715b.
Type not designated.
Original material: Herb. Linn. No. 300.2 (LINN); [icon] in Burman, Thes. Zeylan.: 23, t. 12, f. 2. 1737.
Current name: Wrightia antidysenterica (L.) R. Br. (Apocynaceae).
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 693, DOI: 10.5281/zenodo.291971
title: Evaluation of cortical thickness in bipolar disorder patients using automated software and histogram analysis
Creators: name: Döring, Thomas
Publisher: name: European Congress of Radiology
Year: 2010
Subjects: subject: Computer applications
subject: Computer Applications-General
subject: Computer Applications - Without Subtopic

description: Purpose Methods and Materials Results Conclusion References Personal Information
description: Purpose: Several studies based on Magnetic Resonance Imaging relate morphological brain changes within patients with BD disease in comparison to healthy people, mainly in the frontal lobe (Soares & Mann, 1997; Strakowski, Adler, & DelBello, 2002; Drevets et...
Fock State-enhanced Expressivity of Quantum Machine Learning Models
Creators: name: Gan, Beng Yee
name: Leykam, Daniel
name: Angelakis, Dimitris G.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: Machine Learning (stat.ML)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The data-embedding process is one of the bottlenecks of quantum machine learning, potentially negating any quantum speedups. In light of this, more effective data-encoding strategies are necessary. We propose a photonic-based bosonic data-encoding scheme that embeds classical data points using fewer encoding layers and circumventing the need for nonlinear optical components by mapping the data points into the high-dimensional Fock space. The expressive power of the circuit can be controlled via the number of input photons. Our work shed some light on the unique advantages offers by quantum photonics on the expressive power of quantum machine learning models. By leveraging the photon-number dependent expressive power, we propose three different noisy intermediate-scale quantum-compatible binary classification methods with different scaling of required resources suitable for different supervised classification tasks.
description: 16 pages, 7 figures
Sonnenfleckenzeichnung Nr. 92.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 26.04.1969, 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
An old, metal-rich accreted stellar component in the Milky Way stellar disk
Creators: name: Feuillet, Diane K.
name: Feltzing, Sofia
name: Sahlholdt, Christian
name: Bensby, Thomas
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the possibility that the Milky Way's cool stellar disc includes mergers with ancient stars. Galaxies are understood to form in a hierarchical manner, where smaller (proto-)galaxies merge into larger ones. Stars in galaxies, like the Milky Way, contain in their motions and elemental abundances tracers of past events and can be used to disentangle merger remnants from stars that formed in the main galaxy. The merger history of the Milky Way is generally understood to be particularly easy to study in the stellar halo. The advent of the ESA astrometric satellite Gaia has enabled the detection of completely new structures in the halo such as the Gaia-Enceladus-Sausage. However, simulations also show that mergers may be important for the build-up of the cool stellar disks. Combining elemental abundances for 100 giant branch stars from APOGEE DR17 and astrometric data from Gaia we use elemental abundance ratios to find an hitherto unknown, old stellar component in the cool stellar disk in the Milky Way. We further identify a small sample of RR Lyrae variables with disk kinematics that also show the same chemical signature as the accreted red giant stars in the disk. These stars allows us to date the stars in the accreted component. We find that they are exclusively old.
description: 11 pages, 5 figures, 3 tables, ApJ accepted