cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Kommunikation von Effektstärken und deren Unsicherheit an Lehrer:innen
Creators: name: Schmidt, Kerstin
name: Merk, Samuel
Publisher: name: ZPID (Leibniz Institute for Psychology)
Year: 2024
Subjects: subject: 150

description: Wenn Lehrkräfte evidenzinformiert handeln wollen, stehen sie vor der Herausforderung wissenschaftliche Erkenntnisse finden, interpretieren und bewerten zu müssen, ohne jedoch grundständig sozialwissenschaftlich ausgebildet worden zu sein. Wissenschaftskommunikationsformate wie Clearing Houses, Pressemitteilungen oder Translational Abstracts nehmen sich dieser Herausforderung an, indem sie zum einen bildungswissenschaftliche Studien vorselektieren, teilweise ihre Qualität bewerten und deren Informationen sprachlich und grafisch aufbereiten. Im Vortrag werden verschiedene experimentelle Studien vorgestellt, in welchen zentrale Gelingensbedingungen dieser Aufbereitungen untersucht wurden, wobei der Schwerpunkt auf der Kommunikation von Effektstärken liegt. Dabei wird insbesondere beleuchtet, inwiefern es Lehrkräften gelingt, 1) Effektstärken von inferenzstatistischer Information zu unterscheiden, 2) textuell und grafisch dargestellte Effektstärken akkurat und sensitiv zu interpretieren, aber auch 3) ob diese Akkuratheits- und Sensitivitätseinschätzungen durch Enrichments (z. B. Hervorhebung relevanter Informationen in Effektstärkenvisualisierungen) verbessert werden können.
description: If teachers aim to act in an evidence-informed way, they face the challenge of having to find, interpret and evaluate scientific findings without, however, having received a fundamental training in social sciences. Science communication formats such as clearinghouses, press releases or translational abstracts tackle this challenge by pre-selecting educational science studies, in some cases evaluating their quality, and presenting their information in a text-based and visual manner. In the lecture, various experimental studies will be presented in which central conditions for the success of these presentations were investigated, with a focus on the communication of effect sizes. In particular, it will be examined to what extent teachers are able to 1) differentiate between descriptions of effect sizes and inferential statistical information, 2) interpret text-based and visually presented effect sizes accurately and sensitively, but also 3) whether these accuracy and sensitivity assessments can be improved by enrichments (e.g., by highlighting relevant information in effect size visualizations).
description: Am Mittwoch, den 19. Juni 2024, sprachen Prof. Dr. Samuel Merk und Kirstin Schmidt M.A. vom Institut für Schul- und Unterrichtsentwicklung an der Pädagogischen Hochschule Karlsruhe im ZPID-Kolloquium.
description: On Wednesday, June 19, 2024 Prof. Dr. Samuel Merk and Kirstin Schmidt M.A., Institut für Schul- und Unterrichtsentwicklung at University of Education Karlsruhe gave a talk at the ZPID Colloquium.
Outlier Detection for Multi-Network Data
Creators: name: Dey, Pritam
name: Zhang, Zhengwu
name: Dunson, David B.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Methodology (stat.ME)
subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: It has become routine in neuroscience studies to measure brain networks for different individuals using neuroimaging. These networks are typically expressed as adjacency matrices, with each cell containing a summary of connectivity between a pair of brain regions. There is an emerging statistical literature describing methods for the analysis of such multi-network data in which nodes are common across networks but the edges vary. However, there has been essentially no consideration of the important problem of outlier detection. In particular, for certain subjects, the neuroimaging data are so poor quality that the network cannot be reliably reconstructed. For such subjects, the resulting adjacency matrix may be mostly zero or exhibit a bizarre pattern not consistent with a functioning brain. These outlying networks may serve as influential points, contaminating subsequent statistical analyses. We propose a simple Outlier DetectIon for Networks (ODIN) method relying on an influence measure under a hierarchical generalized linear model for the adjacency matrices. An efficient computational algorithm is described, and ODIN is illustrated through simulations and an application to data from the UK Biobank. ODIN was successful in identifying moderate to extreme outliers. Removing such outliers can significantly change inferences in downstream applications.
description: - 13 page main document, - 5 page supplement - Our method has been implemented in both Python and R and is publicly available at https://www.github.com/pritamdey/ODIN-python and https://www.github.com/pritamdey/ODIN-r - Submitted to Bioinformatics
Limenitidinae Behr 1864
Creators: name: Bland, Keith P.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nymphalidae

description: Limenitidinae
Neptis ADARA Moore, 1878 [1879]
Proceedings of the Zoological Society of London for 1878 (4), 821–859 [830]. Junior subjective synonym of Neptis hylas (Linnaeus, 1758) ssp. kamarupa Moore, 1874 (see Eliot, 1969).
Syntypes, 2 males, 2 females, pinned. Specimen data: Specimen a (male with antennae missing): “Tenasserim” [Handwritten]. “Clive-Bayley | 1913-72 ” [Printed] on verso “ Neptis adara | Moore” [Handwritten by Grimshaw]. “Clive-Bayley | 1936-50 53” on verso “ Neptis adara | Moore? CO-TYPE” [Handwritten (by Grimshaw) on mauve
paper]. Specimen b (male with left antenna missing): “Moulmein to Meetan” [Handwritten]. “Clive-Bayley | 1913- 72 ” [Printed] on verso “ Neptis adara | Moore” [Handwritten by Grimshaw]. “Clive-Bayley | 1936-50 52” on verso “ Neptis adara | Moore?CO-TYPE” [Handwritten (by Grimshaw) on mauve paper]. Specimen c (female with left wing broken and antennae missing): “Moulmein to Meetan”on verso “ ♀ ” [Handwritten]. “ Neptis adara | Moore ♀ ” [Handwritten]. “Clive-Bayley | 1913-72 ” [Printed] on verso “ Neptis adara | Moore” [Handwritten by Grimshaw]. Specimen d (female with tip of right wing and antennae missing): Labels as for Specimen c but species name label absent. Remarks: This material is obviously part of the type series from the Upper Tenasserim Expedition of 1876- 1877.
description: Published as part of Bland, Keith P., 2019, Name-bearing types of butterflies (Lepidoptera, Papilionoidea), in the National Museums of Scotland, Edinburgh, pp. 57-89 in Zootaxa 4559 (1) on pages 76-77, DOI: 10.11646/zootaxa.4559.1.2, http://zenodo.org/record/3522349
Lebadea Felder 1861
Creators: name: Bland, Keith P.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nymphalidae
Lebadea

description: Lebadea ATTENUATA Moore, 1878 [1879]
Proceedings of the Zoological Society of London for 1878 (4), 821–859 [829]. Junior subjective synonym of Lebadea martha martha (Fabricius, 1787) (see D’Abrera, 1984).
Syntypes, 1 male, 1 female, pinned. Specimen data: Specimen reg. no.50 (male, right antenna missing): “Tenasserim” [Handwritten]. “ Lebadea | attenuata Moore” [Handwritten]. “Clive-Bayley | 1913-72 ” [Printed] on verso “ Lebadea | attenuata Moore” [Handwritten]. “Clive-Bayley | 1936-50 50” [Handwritten] on verso “Lebedea attenuata | Moore?CO-TYPE” [Handwritten (by Grimshaw) on mauve paper]. Specimen reg. no.51: Same data as previous specimen only mauve label inscribed “ 1936-50 51.” Remarks: These specimens are obviously part of the type series from the Upper Tenasserim Expedition of 1876-1877.
description: Published as part of Bland, Keith P., 2019, Name-bearing types of butterflies (Lepidoptera, Papilionoidea), in the National Museums of Scotland, Edinburgh, pp. 57-89 in Zootaxa 4559 (1) on page 77, DOI: 10.11646/zootaxa.4559.1.2, http://zenodo.org/record/3522349
The cooling of the Central Compact Object in Cas A from 2006 to 2020
Creators: name: Posselt, B.
name: Pavlov, G. G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report on the study of six Chandra observations (four epochs) of the Central Compact Object (CCO) in the Cassiopeia A supernova remnant with the ACIS instrument in the subarray mode. This mode minimizes spectrum-distorting instrumental effects such as pileup. The data were taken over a time span ~ 14 years. If a non-magnetic carbon atmosphere is assumed for this youngest known CCO, then the temperature change is constrained to be $\dot{T}=-2900\pm 600$ K yr$^{-1}$ or $\dot{T}=-4500\pm 800 $ K yr$^{-1}$ ($1σ$ uncertainties) for constant or varying absorbing hydrogen column density. These values correspond to cooling rates of $-1.5 \pm 0.3$% per 10yr and $-2.3 \pm 0.4$% per 10yr, respectively. We discuss an apparent increase in the cooling rate in the last five years and the variations of the inferred absorbing hydrogen column densities between epochs. Considered together, these changes could indicate systematic effects such as caused by, e.g., an imperfect calibration of the increasing contamination of the ACIS filter.
description: Accepted for publication in ApJ, 6 pages, 2 figures, 2 tables
Sonnenfleckenzeichnung Nr. 105.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 04.05.1966, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1966

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
description: ETH-Bibliothek
Asteroseismology of the multiple stellar populations in the Globular Cluster M4
Creators: name: Tailo, M.
name: Corsaro, E.
name: Miglio, A.
name: Montalbán, J.
name: Brogaard, K.
name: Milone, A. P.
name: Stokholm, A.
name: Casali, G.
name: Bragaglia, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a new asteroseismic analysis of the stars in the Globular Cluster (GC) M4 based on the data collected by the K2 mission. We report the detection of solar-like oscillation in 37 stars, 32 red giant branch (RGB) and 6 red horizontal branch (rHB) stars, the largest sample for this kind of study in GC up to date. Combining information from asteroseismology and multi-band photometry we estimate both the masses and the radii of our targets. Our estimates are in agreement with independent sources, serving as a crucial verification of asteroseismology in the low metallicity regime. As M4 is an old GC, it hosts multiple stellar populations differing in light-element abundances and in helium mass fraction. This generates a mass difference between the populations along the RGB, which in the case of M4 is estimated to be $0.017 M_\odot$. With this wealth of information we can assign population membership and estimate the average mass of the stellar populations, but the current uncertainties do not allow us to resolve this mass difference. The population membership and the seismic data of RGB and HB stars, allow us, however, to assess the integrated mass loss along the RGB of the first generation stars in the cluster. We obtain $\rm ΔM=0.227 \pm0.028 M_\odot$, in good agreement with independent estimates. Finally, we observe the presence of a statistically significant mass-temperature gradient in the rHB stars. This represents the first direct, model-independent observation of the colour-temperature-mass correlation predicted by the theory.
description: 14 pages, 11 figures, 3 tables. Accepted for publication in A&A
Bebearia paludicola Holmes 2001
Creators: name: Bland, Keith P.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nymphalidae
Bebearia
Bebearia paludicola

description: Bebearia paludicola Holmes, 2001 ssp. BLANDI Holmes, 2001
Tropical Zoology 14, 31–62 [48], figure 11. Combination still valid (see Larsen, 2005).
Holotype, male, pinned (abdomen in gelatin capsule); also allotype female, pinned. Specimen data: Specimen a: “ GHANA | Bobiri Forest Reserve | (6 o 41’N, 1 o 20’W) Forest path | M.B.Usher 1.x.1972 | RSM 1973.9 ” [Printed]. “ B.paludicola blandi | Holotype | det. C.W.N. Holmes | Feb.1999 ” [Handwritten (by Holmes) on orange card]. Specimen b: “ GHANA | Mamiri Forest Reserve | 5 o 43’N, 2 o 23’W) | Reserve boundary path [Printed] | Attracted to bananas [Handwritten (by Usher)] | M.B.Usher 28.vii.1975 | RSM 1975.64 ” [Printed]. “ B.paludicola blandi | Allotype | det. C.W.N.Holmes | Feb.1999 ” [Handwritten (by Holmes) on orange card.]. Remarks: These two specimens are unambiguously the holotype and allotype designated by Holmes (2001) and illustrated in Figure 11 (ibidem).
Papilio COCALIA Fabricius, 1793; Holmes, 2001.
Entomologia systematica emendata et aucta 3 (1), 1-488 [250]: Tropical Zoology 14, 31–62 [49], figures 8&9.
Current accepted combination: Bebearia cocalia cocalia (Fabricius, 1793) (see Larsen, 2005).
Neotype, male, pinned: Specimen data: “ Ghana, Mamiri Forest Reserve (5°43’N, 2°23’W), M.B.Usher 11.viii.1975, RSM 1975.64 ” [Printed on white card]. “ B.cocalia, Neotype, des. C.W.N.Holmes, May 2000.” [Handwritten (by Holmes) on orange card]. Remarks: This specimen is without doubt the neotype designated by Holmes (2001) to stabilise the concept of Bebearia cocalia (Fabricius, 1793). It is illustrated in Figures 8 and 9 (ibidem).
description: Published as part of Bland, Keith P., 2019, Name-bearing types of butterflies (Lepidoptera, Papilionoidea), in the National Museums of Scotland, Edinburgh, pp. 57-89 in Zootaxa 4559 (1) on page 77, DOI: 10.11646/zootaxa.4559.1.2, http://zenodo.org/record/3522349
Chromospheric recurrent jets in a sunspot group and their inter-granular origin
Creators: name: Zhao, Jie
name: Su, Jiangtao
name: Yang, Xu
name: Li, Hui
name: Schmieder, Brigitte
name: Ahn, Kwangsu
name: Cao, Wenda
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report on high resolution observations of recurrent fan-like jets by the Goode Solar telescope (GST) in multi-wavelengths inside a sunspot group. The dynamics behaviour of the jets is derived from the Ha line profiles. Quantitative values for one well-identified event have been obtained showing a maximum projected velocity of 42 km s^-1 and a Doppler shift of the order of 20 km s^-1. The footpoints/roots of the jets have a lifted center on the Ha line profile compared to the quiet sun suggesting a long lasting heating at these locations. The magnetic field between the small sunspots in the group shows a very high resolution pattern with parasitic polarities along the inter-granular lanes accompanied by high velocity converging flows (4 km s^-1) in the photosphere. Magnetic cancellations between the opposite polarities are observed in the vicinity of the footpoints of the jets. Along the inter-granular lanes horizontal magnetic field around 1000 Gauss is generated impulsively. Overall, all the kinetic features at the different layers through photosphere and chromosphere favor a convection-driven reconnection scenario for the recurrent fan-like jets, and evidence a site of reconnection between the photosphere and chromosphere corresponding to the inter-granular lanes.
description: to be published in ApJ
An Inquiry Into the Justice of the Peace Courts of Harrison County, West Virginia
Creators: name: Conaway, Jr., Orrin B.
Publisher: name: American University
Year: 2023
Subjects: classificationCode: 44
subject: Human society
classificationCode: 440708
subject: Public administration
classificationCode: 4408
subject: Political science
subject: FOS: Political science

description: Description to be added
Studies of tau neutrino appearance at the DUNE Near Detector complex
Creators: name: Soamasina Herilala Razafinime
Publisher: name: Zenodo
Year: 2022

description: The DUNE experiment will use the new LBNF (Long-Baseline Neutrino Facility) neutrino beam sampled at the Near Detector complex (DUNE ND), 574 m downstream of the production target, and at the Far Detector complex, 1300 km away at the SURF laboratory at a depth of about 1.5 km. The highly capable multi-component Near Detector complex, with a LAr TPC (Liquid Argon Time Projection Chamber) as its primary detector, enables DUNE to probe new physics beyond the Standard Model, including the possibility of short-baseline tau neutrino appearance mediated by sterile neutrino oscillations. Tau neutrino detection is particularly challenging due to the high energy production threshold of the tau lepton and its very short lifetime. However, the excellent spatial resolution of the Near Detector LAr TPC and the large statistics expected (particularly using the high-energy beam configuration) for the LBNF beam provide a unique opportunity to probe these exotic signatures. In this poster, we will present a study of DUNE's projected sensitivities to short-baseline tau neutrino appearance using the DUNE ND and discuss how the sensitivities are enhanced when combining the ND-LAr TPC with downstream components serving as magnetized muon spectrometers, including ND GAr or ND-GAr-Lite, and the SAND detector.
Euphaedra Hübner 1819
Creators: name: Bland, Keith P.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nymphalidae
Euphaedra

description: Euphaedra COOKSONI H. Druce, 1905
Annals & Magazine of Natural History. 7th Series. 16, 549–551 [550–551]. Combination still valid (see Ackery, Smith & Vane-Wright, 1995; Hecq, 1997).
Syntype, male, pinned. Specimen data: “2|1|03” [Handwritten in purple crayon]. “N.W.R.” [Handwritten in ink]. “ Euphaedra | cooksoni | Druce type” [Handwritten in ink] “ Rhodesia | Cookson | 1930-202 | 283” [Printed] on verso “ Euphaedra | cooksoni Druce | TYPE” [Handwritten (by Grimshaw)]. “Not in B.M.” [Handwritten in ink]. “TYPE” [Printed on red paper]. Remarks: This species, named by Herbert Druce (1905), in honour of Mr. Harold Cookson, was described from at least one male and one female. The present specimen from Cookson’s own collection is certainly part of the type series. The species is not included by Gabriel (1927) in the catalogue of types in BM(NH). This, coupled with the presence of the “Type” label (as opposed to “Co-type” label) suggests that Druce meant it as the ‘holotype’. though he did not refer to the specimen as such. There appears to be an error in the type description as the type locality is given as “N.E. Rhodesia ”, which is where Cookson collected most of the material. However the specimen bears a “N. W.R.” label indicating it was taken in North West Rhodesia!
Bebearia cocalioides Hecq, 1988 ssp. HECQI Holmes, 2001
Tropical Zoology 14, 31–62 [46], figures 8 and 9. Combination still valid (see Larsen, 2005).
Holotype, male, pinned (genitalia on slide CWNH 13): also allotype female (genitalia on slide CWNH 25). Specimen data: 1887 specimen: “Camaroons [sic]. [Printed] | 1887-1” [Handwritten]. “ Bebearia | mardania gp. | sl[ide]. CWNH (13)” [Printed]. “ B. cocalioides hecqi | Holotype | det. C.W.N.Holmes | Feb. 1999 ” [Handwritten (by Holmes) on orange card]. 1888 specimen: “ Cameroons. | 1888.97.1. [Printed] | 75” [Handwritten]. “ Bebearia | mardania gp. | sl[ide]. CWNH (25)” [Printed]. “ B. cocalioides heqi [sic] | Allotype | det. C.W.N.Holmes | Feb. 1999 ” [Handwritten (by Holmes) on orange card]. Remarks: These two specimens are unambiguously the holotype and allotype designated by Holmes (2001), and illustrated in Figures 8 and 9 (ibidem).
description: Published as part of Bland, Keith P., 2019, Name-bearing types of butterflies (Lepidoptera, Papilionoidea), in the National Museums of Scotland, Edinburgh, pp. 57-89 in Zootaxa 4559 (1) on pages 77-78, DOI: 10.11646/zootaxa.4559.1.2, http://zenodo.org/record/3522349
Depletion of Moderately Volatile Elements by Open-System loss in the Early Solar Nebula
Creators: name: Sengupta, Debanjan
name: Estrada, Paul R.
name: Cuzzi, Jeffrey N.
name: Humayun, Munir
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: Rocky bodies of the inner solar system display a systematic depletion of the "Moderately Volatile Elements" (MVEs) that correlates with the expected condensation temperature of their likely host materials under protoplanetary nebula conditions. In this paper, we present and test a new hypothesis in which open system loss processes irreversibly remove vaporized MVEs from high nebula altitudes, leaving behind the more refractory solids residing much closer to the midplane. The MVEs irreversibly lost from the nebula through these open system loss processes are then simply unavailable for condensation onto planetesimals forming even much later, after the nebula cooled, overcoming a critical difficulty encountered by previous models of this type. We model open system loss processes operating at high nebula altitudes, such as resulting from disk winds flowing out of the system entirely, or layered accretion directly onto the young sun. We find that mass loss rates higher than found in typical T-Tauri disk winds, lasting short periods of time, are most satisfactory, pointing to multiple intense early outburst stages. Using our global nebula model, incorporating realistic particle growth and inward drift for solids, we constrain how much the MVE depletion signature in the inner region is diluted by the drift of undepleted material from the outer nebula. We also find that a significant irreversible loss of the common rock-forming elements (Fe, Mg, Si) can occur, leading to a new explanation of another longstanding puzzle of the apparent "enhancement" in the relative abundance of highly refractory elements in chondrites.
description: 35 pages, 16 figures, Accepted for publication in The Astrophysical Journal
Hard X-ray emission in Centaurus A
Creators: name: Rani, B.
name: Mundo, S. A.
name: Mushotzky, R.
name: Lien, A. Y.
name: Gurwell, M. A.
name: Kim, J. Y.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We used 13 years of Swift/BAT observations to probe the nature and origin of hard X-ray (14-195 KeV) emission in Centaurus A. Since the beginning of the Swift operation in 2004, significant X-ray variability in the 14-195 KeV band is detected, with mild changes in the source spectrum. Spectral variations became more eminent after 2013, following a softer-when-brighter trend. Using the power spectral density method, we found that the observed hard X-ray photon flux variations are consistent with a red-noise process of slope, $-1.3$ with no evidence for a break in the PSD. We found a significant correlation between hard X-ray and 230 GHz radio flux variations, with no time delay longer than 30 days. The temporal and spectral analysis rules out the ADAF (advection-dominated accretion flow) model, and confirms that the hard X-ray emission is produced in the inner regions of the radio jet.
description: Accepted for publication in ApJ
Over seven decades of solar microwave data obtained with Toyokawa and Nobeyama Radio Polarimeters
Creators: name: Shimojo, Masumi
name: Iwai, Kazumasa
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Monitoring observations of solar microwave fluxes and their polarization began in Japan during the 1950s at Toyokawa and Mitaka. At present (April 2022), monitoring observations continue with the Nobeyama Radio Polarimeters (NoRP) at the Nobeyama campus of the National Astronomical Observatory of Japan (NAOJ). In this paper, we present a brief history of the solar microwave monitoring observations preceding those now carried out by NoRP. We then review the solar microwave obtained at Toyokawa and Nobeyama and their metadata. The datasets are publicly provided by the Solar Data Archive System (SDAS) operated by the Astronomy Data Center of the NAOJ, via http (https://solar.nro.nao.ac.jp/norp/) and FTP (ftp://solar-pub.nao.ac.jp/pub/nsro/norp/) protocols.
description: 29 pages, 12 figures, accepted to Geoscience Data Journal
Bebearia orientis
Creators: name: Bland, Keith P.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nymphalidae
Bebearia
Bebearia orientis

description: Bebearia orientis (Karsch, 1985) ssp. MALAWIENSIS Holmes, 2001
Tropical Zoology 14, 31 – 62 [56 – 57], figures 8 and 9. Combination still valid (see Kunz, 2016).
Holotype, male, pinned (half of right antenna missing); also allotype female and paratypes 3 males, 1 female, all pinned (abdomen of allotype on slide CWNH.30). Specimen data: Specimen a: “Vizara. 2100’ 3.v.62 ” [Handwritten (by Gifford)] in blue ink on greaseproof paper]. “B. orientalis | malawiensis | Holotype | det. C.W.N. Holmes | Feb.1999 ” [Handwritten (by Holmes) on orange card]. Specimen b: “Vizara. | 2100’ | Raphia swamp forest | 11.v.62 ” [Handwritten (by Gifford) in blue ink on greaseproof paper]. “ Bebearia | mardania gp. | sl[ide]. CWNH (30)” [Printed]. “B.orientalis | malawiensis | Allotype | det. C.W.N.Holmes | Feb. 1999 ” [Handwritten (by Holmes) on orange card]. Specimen c (♂) “Lauderdale Estate, Mlanje, 11.vi.61 ” [Handwritten (by Gifford)]. “ D.R.Gifford, RSM 1962.66 ” [Printed]. Specimens d (♂) and e (♀) labelled same as specimen c but dated “ 21.v.61.” Specimen f (♂): “Malanji, Brit.C.Africa ” [Handwritten]. “Adams Bequest, B.M. 1912.399, R.S.M. 1969.” [Printed]. Remarks: These six specimens are unambiguously the holotype, allotype and 4 paratypes designated by Holmes (2001), and illustrated in Figures. 8 and 9 of that paper.
Bebearia MARDANIA (Fabricius, 1793); Holmes, 2001.
Tropical Zoology 14, 31–62 [45], figures 2, 8 and 9.
Neotype, female, pinned: Specimen data: “ Ghana, Tano Nimri Forest Reserve (5°45’N, 2°36’W, M.B.Usher 3.viii.1975, RSM 1975.64” [Printed on white card]. “ B.mardania. Neotype, des. C.W.N.Holmes, May 2000 ” [Handwritten (by Holmes) on orange card]. Remarks: This specimen is unambiguously the neotype described by Holmes to stabilise the concept of B.mardania (Fabricius, 1793) (Holmes, 2001). It is figured in Figure 2,8,& 9 of Holmes (2001).
description: Published as part of Bland, Keith P., 2019, Name-bearing types of butterflies (Lepidoptera, Papilionoidea), in the National Museums of Scotland, Edinburgh, pp. 57-89 in Zootaxa 4559 (1) on page 78, DOI: 10.11646/zootaxa.4559.1.2, http://zenodo.org/record/3522349
Pseudostreamer influence on flux rope evolution
Creators: name: Sahade, A.
name: Cécere, M.
name: Sieyra, M. V.
name: Krause, G.
name: Cremades, H.
name: Costa, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A critical aspect of solar activity is the coupling between eruptions and the surrounding coronal magnetic field, which determines the trajectory and morphology of the eruptive event. Pseudostreamers (PSs) are coronal magnetic structures formed by arcs of twin loops capped by magnetic field lines from coronal holes of the same polarity that meet at a central spine. They contain a single magnetic null point in the spine, potentially influencing the evolution of nearby flux ropes (FRs). To understand the net effect of the PS on FR eruptions is first necessary to study diverse and isolated FR-PS scenarios, which are not influenced by other magnetic structures. We performed numerical simulations in which a FR structure is in the vicinity of a PS magnetic configuration. The combined magnetic field of the PS and the FR results in the formation of two magnetic null points. We evolve this scenario by numerically solving the magnetohydrodynamic equations in 2.5D. The simulations consider a fully ionised compressible ideal plasma in the presence of a gravitational field and a stratified atmosphere. We find that the dynamic behaviour of the FR can be categorised into three different classes based on the FR trajectories and whether it is eruptive or confined. Our analysis indicates that the magnetic null points are decisive in the direction and intensity of the FR deflection and their hierarchy depends on the topological arrangement of the scenario. Moreover, the PS lobe acts as a magnetic cage enclosing the FR. We report that the total unsigned magnetic flux of the cage is a key parameter defining whether the FR is ejected or not.
The Proper Motion of the Pulsar J1124-5916 in the Galactic Supernova Remnant G292.0+1.8
Creators: name: Long, Xi
name: Patnaude, Daniel J.
name: Plucinsky, Paul P.
name: Gaetz, Terrance J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the first direct measurement of the proper motion of pulsar J1124-5916 in the young, oxygen-rich supernova remnant G292.0+1.8. Using deep Chandra ACIS-I observations from 2006 and 2016, we measure a positional change of $0.^{\prime\prime}21$ $\pm$ $0.^{\prime\prime}05$ over the $\sim$ 10 year baseline, or $\sim$ $0.^{\prime\prime}02$ yr$^{-1}$. At a distance of 6.2 $\pm$ 0.9 kpc, this corresponds to a kick velocity in the plane of the sky of $\mathrm{612\pm 152\,km \, s^{-1}}$. We compare this direct measurement against the velocity inferred from estimates based on the center of mass of the ejecta. Additionally, we use this new proper motion measurement to compare the motion of the neutron star to the center of expansion of the optically emitting ejecta. We derive an age estimate for the supernova remnant of $\gtrsim$ 2000 years. The high measured kick velocity is in line with recent studies of high proper motion neutron stars in other Galactic supernova remnants, and consistent with a hydrodynamic origin to the neutron star kick.
description: Accepted for publication in ApJ, 15 pages, 12 figures, 6 tables
British Gallup Poll: CQ 038A
Creators: name: Social Surveys (Gallup Poll) Limited
Publisher: name: Roper Center for Public Opinion Research
Year: 1996

description: Government approval rating(1); Thatcher approval rating(1); political party leaders(2); political party(2); 1987 election(2); price increase(4); economic situation(2); wages(2); Iraq's economic blockade(8); Gulf miltary action(5); Gulf crisis(4).
Sonnenfleckenzeichnung Nr. 45.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.02.1966, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1966

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
description: ETH-Bibliothek
O cálculo do custo de doenças
Creators: name: Amil Dias, Jorge
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: O conhecimento do custo exacto envolvido na prestação de cuidados de saúde é importantíssimo para se avaliar o custo/ benefício de novas intervenções, tratamentos, prevenções, etc. Claro que na doença há sempre valores não quantificáveis – estar doente é só por si um dano considerável para o próprio e para os familiares independentemente do preço do tratamento – mas não pode ignorar-se o esforço financeiro que a Sociedade investe no tratamento ou prevenção da doença de cada um dos seus cidadãos.
description: Portuguese Journal of Pediatrics, Vol 38 No 4 (2007)
Bebearia paludicola Holmes 2001
Creators: name: Bland, Keith P.
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Nymphalidae
Bebearia
Bebearia paludicola

description: Bebearia PALUDICOLA Holmes, 2001
Tropical Zoology 14, 31–62 [47–48], figure 10. Combination still valid (see Larsen, 2005).
Holotype, male, pinned (abdomen in gelatine capsule); also allotype, female, pinned. Specimen data: Specimen a: “Bitje, | Ja River, | Cameroons ” [Printed]. “Adams Bequest | B.M. 1912-399 | R.S.M. 1969. 20” [Printed]. “ B. paludicola paludicola | Holotype | det. C.W.N. Holmes | Feb. 1999 ” [Handwritten (by Holmes) on orange card]. Specimen b: “Bitje, Ja River, | Cameroons ” [Printed]. “Adams Bequest | B.M. 1912-399 | R.S.M. 1969.20” [Printed]. “ Bebearia | mardania gp. | sl[ide]. CWNH (28)” [Printed]. “ B.paludicola paludicola | Allotype | det. C.W.N. Holmes | Feb. 1999 ” [Handwritten (by Holmes) on orange card]. Remarks: These two specimens are unambiguously the holotype and allotype designated by Holmes (2001), and illustrated in Figure 10 (ibidem).
description: Published as part of Bland, Keith P., 2019, Name-bearing types of butterflies (Lepidoptera, Papilionoidea), in the National Museums of Scotland, Edinburgh, pp. 57-89 in Zootaxa 4559 (1) on page 78, DOI: 10.11646/zootaxa.4559.1.2, http://zenodo.org/record/3522349
Sítio da SPP na Internet com acreditação  internacional de qualidade
Creators: name: Coelho, Mário
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: Após um rigoroso e demorado processo de reformulação, em Agosto de 2007 o sítio (web) da Sociedade Portuguesa de Pediatria na internet (www.spp.pt) obteve a certificação de qualidade conferida pelo projecto Webs Médicas de Calidad (pWMC) e passará a exibir o símbolo dessa distinção na sua página de entrada.

O projecto Webs Médicas de Calidad é uma iniciativa na internet que tem como objectivo a melhoria da qualidade das webs dedicadas à saúde humana. Este símbolo confirma que os sítios da Internet certificados passaram por um rigoroso processo de avaliação e estão sujeitos a procedimentos de auditoria externa periódica com a finalidade de verificar que são cumpridos continuamente o código de conduta, os princípios éticos e os critérios de qualidade próprios da pWMC (www.pwmc.org).
description: Portuguese Journal of Pediatrics, Vol 38 No 4 (2007)
Biblioteca da Pediatria Portuguesa e Biblioteca Internacional da SPP
Creators: name: Coelho, Mário
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: A Sociedade Portuguesa de Pediatria iniciou, há cerca de oito anos, sob as presidências sucessivas dos Drs. João Calheiros Lobo, Libério Ribeiro e Manuel Gonçalo Cordeiro Ferreira, a organização do seu espólio científico e bibliográfico pediátrico em três áreas bibliográficas principais: a “Biblioteca da Pediatria Portuguesa”, dedicada a textos científicos pediátricos de autores portugueses; a “Biblioteca Internacional da SPP” que inclui obras científicas essencialmente pediátricas, mas em língua estrangeira; e, acessoriamente, uma área de “Programas, folhetos e cartazes” de reuniões promovidas pela SPP e suas Secções.
description: Portuguese Journal of Pediatrics, Vol 38 No 4 (2007)
Unveiling the veil of workplace Loneliness: A Theory-Concept-Methodology (TCM) framework
Creators: name: Choudhary, Mohammadamin
name: Jena, Biswa Prakash
name: Patre, Smruti
Publisher: name: Psychology Hub
Year: 2024

description: The aim of the study is to learn more about the causes and effects of workplace loneliness. The study uses a TCM (Theory, Context, Methodology) framework based on various studies to critically assess and analyse the existing body of research on workplace loneliness from 2010 to 2021. This paper tries to do a comprehensive review of the antecedents, underlying processes, and outcomes, which will provide future directions for further development of the workplace loneliness construct and identify significant opportunities for researchers to advance the field's theoretical and empirical development.
description: Psychology Hub, Vol. 41 No. 1 (2024)
A search for two-component Majorana dark matter in a simplified model using the full exposure data of PandaX-II experiment
Creators: name: Yuan, Ying
name: Abdukerim, Abdusalam
name: Bo, Zihao
name: Chen, Wei
name: Chen, Xun
name: Chen, Yunhua
name: Cheng, Chen
name: Cui, Xiangyi
name: Fan, Yingjie
name: Fang, Deqing
name: Fu, Changbo
name: Fu, Mengting
name: Geng, Lisheng
name: Giboni, Karl
name: Gu, Linhui
name: Guo, Xuyuan
name: Han, Ke
name: He, Changda
name: He, Jinrong
name: Huang, Di
name: Huang, Yanlin
name: Huang, Zhou
name: Hou, Ruquan
name: Ji, Xiangdong
name: Ju, Yonglin
name: Li, Chenxiang
name: Li, Mingchuan
name: Li, Shu
name: Li, Shuaijie
name: Lin, Qing
name: Liu, Jianglai
name: Lu, Xiaoying
name: Luo, Lingyin
name: Ma, Wenbo
name: Ma, Yugang
name: Mao, Yajun
name: Meng, Yue
name: Shaheed, Nasir
name: Ning, Xuyang
name: Qi, Ningchun
name: Qian, Zhicheng
name: Ren, Xiangxiang
name: Shang, Changsong
name: Shen, Guofang
name: Si, Lin
name: Sun, Wenliang
name: Tan, Andi
name: Tao, Yi
name: Wang, Anqing
name: Wang, Meng
name: Wang, Qiuhong
name: Wang, Shaobo
name: Wang, Siguang
name: Wang, Wei
name: Wang, Xiuli
name: Wang, Zhou
name: Wu, Mengmeng
name: Wu, Weihao
name: Xia, Jingkai
name: Xiao, Mengjiao
name: Xiao, Xiang
name: Xie, Pengwei
name: Yan, Binbin
name: Yan, Xiyu
name: Yang, Jijun
name: Yang, Yong
name: Yu, Chunxu
name: Yuan, Jumin
name: Zhang, Dan
name: Zhang, Minzhen
name: Zhang, Peng
name: Zhang, Tao
name: Zhao, Li
name: Zheng, Qibin
name: Zhou, Jifang
name: Zhou, Ning
name: Zhou, Xiaopeng
name: Zhou, Yong
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the two-component Majorana dark matter model, one dark matter particle can scatter off the target nuclei, and turn into a slightly heavier component. In the framework of a simplified model with a vector boson mediator, both the tree-level and loop-level processes contribute to the signal in direct detection experiment. In this paper, we report the search results for such dark matter from PandaX-II experiment, using total data of the full 100.7 tonne$\cdot$day exposure. No significant excess is observed, so strong constraints on the combined parameter space of mediator mass and dark matter mass are derived. With the complementary search results from collider experiments, a large range of parameter space can be excluded.
The importance of black hole repositioning for galaxy formation simulations
Creators: name: Bahé, Yannick M.
name: Schaye, Joop
name: Schaller, Matthieu
name: Bower, Richard G.
name: Borrow, Josh
name: Chaikin, Evgenii
name: Kugel, Roi
name: Nobels, Folkert
name: Ploeckinger, Sylvia
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Active galactic nucleus (AGN) feedback from accreting supermassive black holes (SMBHs) is an essential ingredient of galaxy formation simulations. The orbital evolution of SMBHs is affected by dynamical friction that cannot be predicted self-consistently by contemporary simulations of galaxy formation in representative volumes. Instead, such simulations typically use a simple "repositioning" of SMBHs, but the effects of this approach on SMBH and galaxy properties have not yet been investigated systematically. Based on a suite of smoothed particle hydrodynamics simulations with the SWIFT code and a Bondi-Hoyle-Lyttleton subgrid gas accretion model, we investigate the impact of repositioning on SMBH growth and on other baryonic components through AGN feedback. Across at least a factor ~1000 in mass resolution, SMBH repositioning (or an equivalent approach) is a necessary prerequisite for AGN feedback; without it, black hole growth is negligible. Limiting the effective repositioning speed to $\lesssim$ 10 km/s delays the onset of AGN feedback and severely limits its impact on stellar mass growth in the centre of massive galaxies. Repositioning has three direct physical consequences. It promotes SMBH mergers and thus accelerates their initial growth. In addition, it raises the peak density of the ambient gas and reduces the SMBH velocity relative to it, giving a combined boost to the accretion rate that can reach many orders of magnitude. Our results suggest that a more sophisticated and/or better calibrated treatment of SMBH repositioning is a critical step towards more predictive galaxy formation simulations.
description: 17 pages, 11 figures (including appendix); accepted by MNRAS. Minor updates to match accepted version
Adolescentes, sexo e telemóveis
Creators: name: Nodin, Nuno
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: Veio recentemente a público que alguns adolescentes portugueses trocariam favores sexuais através da Internet por dinheiro ou por carregamentos de telemóvel. Esta notícia surge na sequência da publicação do trabalho de dois professores que observaram diversas chat-rooms frequentadas por adolescentes e onde verificaram diversos comportamentos desse tipo (Montalvo & Monteiro, 2007). A notícia surge envolta numa aura de escândalo e de indignação, mais uma vez demonizando-se a Internet e atribuindo-lhe alguma da responsabilidade no fenómeno. Aquestão é que não se trata de um fenómeno novo nem tão pouco se poderão atribuir à Internet responsabilidades directas no sucedido.
description: Portuguese Journal of Pediatrics, Vol 38 No 4 (2007)
Factores preditivos de cicatriz renal após pielonefrite em crianças com menos de dois anos de idade
Creators: name: Pimentel, Sónia
name: Figueiredo, António
name: Oliveira, Laura
name: Varandas, Luís
Publisher: name: Portuguese Journal of Pediatrics
Year: 2014

description: Objectivos: Identificar factores laboratoriais e imagiológicos associados ao desenvolvimento de cicatriz renal sequelar após pielonefrite em doentes com menos de dois anos de idade e avaliar o papel da ecografia no estudo não invasivo de pielonefrite. Local. Hospital pediátrico universitário de nível III. População. Crianças com idade inferior a dois anos hospitalizadas com o diagnóstico de primeira pielonefrite.

Métodos: Avaliação prospectiva do risco de cicatriz renal, através de parâmetros laboratoriais e imagiológicos. Estudo de efectividade da ecografia renal e vesical para identificar pielonefrite aguda e refluxo vesico-ureteral (RVU). Admite-se como método padrão para detecção de pielonefrite aguda e cicatriz renal a cintigrafia renal com DMSA e para detecção de RVU, a cisto-uretografia permiccional (CUM).

Resultados: Estudaram-se 134 crianças, com mediana de idades de 3 meses (p25-p75: 1-9 meses) sendo 60% do sexo masculino. Acintigrafia em ambulatório evidenciou a presença de cicatriz renal em 42% das crianças. Valores de proteína C reactiva superiores a 5 mg/dl estiveram associados a alterações da cintigrafia em ambulatório [RR 2,7 (IC95% 1,1-7), VP+ 64,3%, VP– 76,5%]. A presença de RVU grau ≥ II esteve associada a cicatriz renal na cintigrafia em ambulatório [RR 2,6 (IC95% 1,7-4,2), VP+ 100%, VP– 51,7%]. Vinte por cento das crianças tinha RVU verificado pela CUM, tendo a ecografia excluído de forma significativa a sua presença, em relação à CUM [LR+ 9,9 (1,4-69,3), VP– 94,4%].

Conclusões: No grupo estudado, o valor de proteína C reactiva e a presença de RVU grau ≥ II foram os principais factores preditivos de cicatriz renal. O papel da ecografia parece ser relevante no estudo de pielonefrite, sobretudo para excluir RVU.
description: Portuguese Journal of Pediatrics, Vol 38 No 4 (2007)
Out-of-equilibrium dynamics arising from slow round-trip variations of Hamiltonian parameters across quantum and classical critical points
Creators: name: Tarantelli, Francesco
name: Vicari, Ettore
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We address the out-of-equilibrium dynamics of many-body systems subject to slow time-dependent round-trip protocols across quantum and classical (thermal) phase transitions. We consider protocols where one relevant parameter w is slowly changed across its critical point wc = 0, linearly in time with a large time scale ts, from wi < 0 to wf > 0 and then back to wi < 0, thus entailing multiple passages through the critical point. Analogously to the one-way Kibble-Zurek protocols across a critical point, round-trip protocols develop dynamic scaling behaviors at both classical and quantum transitions, put forward within renormalization-group frameworks. The scaling scenario is analyzed within some paradigmatic models undergoing quantum and classical transitions belonging to the two-dimensional Ising universality class, such as one-dimensional quantum Ising models and fermionic wires, and two-dimensional classical Ising models (supplemented with a purely relaxational dynamics). While the dynamic scaling frameworks are similar for classical and quantum systems, substantial differences emerge due to the different nature of their dynamics, which is purely relaxational for classical systems (implying thermalization in the large-time limit at fixed model parameters), and unitary in the case of quantum systems. In particular, when the critical point separates two gapped (short-ranged) phases and the extreme value wf > 0 is kept fixed in the large-ts limit of the round-trip protocol, we observe hysteresis-like scenarios in classical systems, while quantum systems do not apparently develop a sufficiently robust scaling limit along the return way, due to the presence of rapidly oscillating relative phases among the relevant quantum states.
description: 24 pages, Phys. Rev. B in press