cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
Creators: name: Zeng, Yaotian
name: Liu, Zheng-Wei
name: Meng, Xiangcun
name: Han, Zhanwen
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: Recent studies have suggested that type Iax supernovae (SNe Iax) are likely to result from a weak deflagration explosion of a Chandrasekhar-mass white dwarf in a binary system with a helium (He)-star companion. Assuming that most SNe Iax are produced from this scenario, in this work we extend our previous work on the three-dimensional hydrodynamical simulation of ejecta-companion interaction by taking the orbital and spin velocities of the progenitor system into account. We then follow the post-impact evolution of a surviving He-star companion by using the one-dimensional stellar evolution code \textsc{MESA}. We aim to investigate the post-explosion rotation properties of a He-star companion in SNe Iax. We find that the He-star companion spins down after the impact due to the angular-momentum loss and expansion caused by the mass-stripping and shock heating during the interaction. This leads to the situation where the surface rotational speed of the surviving companion can drop to one-third of its pre-explosion value when it expands to a maximum radius a few years after the impact. Subsequently, the star shrinks and spins up again once the deposited energy is released. This spin-switching feature of the surviving He-star companions of SNe Iax may be useful for the identification of such objects in future observations.
description: 12 pages, 6 figures, accepted for publication in Research in Astronomy and Astrophysics
Parariukiaria kabaki Golovatch 2014, comb. nov.
Creators: name: Nguyen, Anh D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Diplopoda
Polydesmida
Xystodesmidae
Parariukiaria
Parariukiaria kabaki

description: Parariukiaria kabaki (Golovatch, 2014) comb. nov.
Riukiaria kabaki Golovatch, 2014: 196, figs 23–29.
Remarks. This third species was also described from Sichuan Province (China). The species is diagnosed by gonopod coxa with a seta; the prefemoral process is very short, stout and erect spiniform; the solenomere is long and bifurcate at the distal part, both branches acuminate towards tip (Golovatch, 2014). Those characters place species into Parariukiaria.
description: Published as part of Nguyen, Anh D., 2016, Discovery of a new millipede species in northern Vietnam, and the proposal of a new genus, Parariukiaria (Diplopoda, Polydesmida, Xystodesmidae), pp. 331-336 in Zootaxa 4121 (3) on page 335, DOI: 10.11646/zootaxa.4121.3.7, http://zenodo.org/record/257159
Additional file 1 of Intention to seek emergency medical services during community overdose events in British Columbia, Canada: a cross-sectional survey
Creators: name: Kievit, Bradley
name: Xavier, Jessica C.
name: Ferguson, Max
name: Palis, Heather
name: Moallef, Soroush
name: Slaunwhite, Amanda
name: Gillis, Terri
name: Virk, Rajmeet
name: Buxton, Jane A.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. Good Samaritan Drug Overdose Act Survey. Survey questions asked to respondents either in-person or online.
On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4-2807
Creators: name: Sanna, A.
name: Burderi, L.
name: Di Salvo, T.
name: Riggio, A.
name: Altamirano, D.
name: Marino, A.
name: Bult, P.
name: Strohmayer, T. E.
name: Guillot, S.
name: Malacaria, C.
name: Ng, M.
name: Mancuso, G.
name: Mazzola, S. M.
name: Albayati, A. C.
name: Iaria, R.
name: Manca, A.
name: Cabras, C.
name: Anitra, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4-2807 monitored by NICER and XMM-Newton during its latest outburst after almost eleven years of quiescence. From the coherent timing analysis of the pulse profiles, we updated the orbital ephemerides of the system. Large phase jumps of the fundamental frequency phase of the signal are visible during the outburst, consistent with what was observed during the previous outburst. Moreover, we report on the marginally significant evidence for non-zero eccentricity ($e\simeq 4\times 10^{-5}$) obtained independently from the analysis of both the 2021 and 2010 outbursts and we discuss possible compatible scenarios. Long-term orbital evolution of SWIFT J1749.4-2807 suggests a fast expansion of both the NS projected semi-major axis $(x)$, and the orbital period $(P_{\rm orb})$, at a rate of $\dot{x}\simeq 2.6\times 10^{-13}\,\text{lt-s}\,\text{s}^{-1}$ and $\dot{P}_{\rm orb}\simeq 4 \times 10^{-10}\,\text{s}\,\text{s}^{-1}$, respectively. SWIFT J1749.4-2807 is the only accreting millisecond X-ray pulsar, so far, from which the orbital period derivative has been directly measured from appreciable changes on the observed orbital period. Finally, no significant secular deceleration of the spin frequency of the compact object is detected, which allowed us to set a constraint on the magnetic field strength at the polar caps of $B_{PC}<1.3\times 10^{8}~\text{G}$, in line with typical values reported for AMXPs.
description: 13 pages, 3 figures, 1 table. Accepted for publication in MNRAS
Parariukiaria
Creators: name: Nguyen, Anh D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Diplopoda
Polydesmida
Xystodesmidae
Parariukiaria

description: Key to species of the genus Parariukiaria
1 The leg prefemora entirely without ventral spines. Gonopod prefemoral process absent...................... P. korolevi
- The leg prefemora with ventral spines. Gonopod prefemoral process present...................................... 2
2 Gonopod coxa without a macroseta. Gonopod prefemoral process short, small, but strong, curved, tuberculiform P. belousovi
- Gonopod coxa with a macroseta. Gonopod prefemoral process small, triangular................................... 3
3 Solenomere slender, extremely long, curved.................................................... P. cucfuongensis
- Solenomere bifurcate and flagelliform.............................................................. P. kabaki
description: Published as part of Nguyen, Anh D., 2016, Discovery of a new millipede species in northern Vietnam, and the proposal of a new genus, Parariukiaria (Diplopoda, Polydesmida, Xystodesmidae), pp. 331-336 in Zootaxa 4121 (3) on page 335, DOI: 10.11646/zootaxa.4121.3.7, http://zenodo.org/record/257159
Estimating accurate reddening values of LAMOST M dwarfs
Creators: name: Shen, Han
name: Chen, Bingqiu
name: Guo, Helong
name: Yuan, Haibo
name: Sun, Weixiang
name: Li, Jing
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: M dwarfs are the dominating type of stars in the solar neighbourhood. They serve as excellent tracers for the study of the distribution and properties of the nearby interstellar dust. In this work, we aim to obtain high accuracy reddening values of M dwarf stars from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 8 (DR8). Combining the LAMOST spectra with the high-quality optical photometry from the Gaia Early Data Release 3 (Gaia EDR3), we have estimated the reddening values $E(G_{\rm BP}-G_{\rm RP})$ of 641,426 M dwarfs with the machine-learning algorithm Random Forest regression. The typical reddening uncertainty is only 0.03 mag in $E(G_{\rm BP}-G_{\rm RP})$. We have obtained the reddening coefficient $R_{(G_{\rm BP}-G_{\rm RP})}$, which is a function of the stellar intrinsic colour $(G_{\rm BP}-G_{\rm RP})_0$ and reddening value $E(B-V)$. The values of $E(B-V)$ are also provided for the individual stars in our catalogue. Our resultant high accuracy reddening values of M dwarfs, combined with the Gaia parallaxes, will be very powerful to map the fine structures of the dust in the solar neighbourhood.
description: 8 pages, 8 figures, accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 3624.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.04.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 1853 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
title: How to Conduct Cognitive Interviews in Times of COVID-19
Creators: name: Lenzner, Timo
name: Hadler, Patricia
name: Neuert, Cornelia
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2021
Subjects: subject: Pretesting
subject: Covid-19
subject: Remote Interviewing
subject: Survey Methodology
subject: Cognitive Interviewing

description: The outbreak of COVID-19 has created new challenges for face-to-face research activities, including conducting in-person cognitive interviews. The first lockdown in Germany in mid-March 2020 coincided with the preparation phase of a pretest that we planned to conduct face-to-face in our pretest lab in Mannheim. Since we were no longer able to interview participants in person, we quickly had to come up with alternative ways of conducting pretests without simply switching to the online mode and testing the questionnaires via web probing. This blog post tells the story of how we switched to remote cognitive interviewing and reflects the experience we have gathered with this method over the last 12 months.
description: Der Ausbruch von COVID-19 hat Face-to-Face-Forschungsaktivitäten vor neue Herausforderungen gestellt, einschließlich der Durchführung von persönlichen kognitiven Interviews. Der erste Lockdown in Deutschland Mitte März 2020 fiel direkt in die Vorbereitungsphase eines Pretests, im Zuge dessen wir persönlich-mündliche Interviews in unserem Pretest-Labor in Mannheim durchführen wollten. Da es uns nicht mehr möglich war, Testpersonen persönlich zu befragen, mussten wir kurzfristig auf alternative Wege der Durchführung von Pretests umsteigen, ohne jedoch einfach nur in den Online-Modus zu wechseln und die Fragebögen mittels Web Probing zu testen. Dieser Blog-Beitrag erzählt, wie wir auf Kognitive Remote Interviews umgestiegen sind, und reflektiert unsere Erfahrungen, die wir in den letzten zwölf Monaten mit dieser Methode gesammelt haben.
description: GESIS Blog
L’Italia o l’invenzione della letteratura spagnola. Frenching Amadis. Stampa e orizzonte europeo. Ancora traduzioni. I viaggi di Diana. Picari pellegrini
Creators: name: Cabo Aseguinolaza, Fernando
name: Bognolo, Anna
Publisher: name: Historias Fingidas
Year: 1970

description: Traduzione di alcune pagine di Fernando Cabo Aseguinolaza pubblicate originariamente in El lugar de la literatura española, vol. 9 di Historia de la literatura española, diretta da José-Carlos Mainer, Barcelona, Editorial Crítica, 2012, pp. 106-144. In particolare si traducono i seguenti paragrafi: «Italia o la invención de la literatura española», «Frenching Amadis», «Imprenta y horizonte europeo», «Más traducciones», «Los viajes de Diana», «Pícaros peregrinos». Italian translation of some essays on Spanish literature by Fernando Cabo Aseguinolaza, originally published in El lugar de la literatura española, vol. 9 of Historia de la literatura española, directed by José-Carlos Mainer, Barcelona, Editorial Crítica, 2012, pp. 106-144. Keywords: Fernando Cabo Aseguinolaza, Italian translation, Historia de la literatura española, El lugar de la literatura española, Spanish literature in Europe, print culture, Renaissance, Siglo de Oro, literary relations.
description: Historias Fingidas, No. 1 (2013)
Additional file 2 of Intention to seek emergency medical services during community overdose events in British Columbia, Canada: a cross-sectional survey
Creators: name: Kievit, Bradley
name: Xavier, Jessica C.
name: Ferguson, Max
name: Palis, Heather
name: Moallef, Soroush
name: Slaunwhite, Amanda
name: Gillis, Terri
name: Virk, Rajmeet
name: Buxton, Jane A.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Supplemental Figure and Table. A concept map of the variables used to inform multivariable model construction and a table comparing the final regression model block generated by complete case analysis vs. multiple imputation.
Sonnenfleckenzeichnung Nr. 3732.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 16.08.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 1955 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
Emerging Two-Dimensional Magnetism in Nonmagnetic Electrides Hf2X (X = S, Se, Te)
Creators: name: Liu, Shuyuan
name: Wang, Chongze
name: Jeon, Hyunsoo
name: Yu, Jia
name: Cho, Jun-Hyung
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Recent experimental discoveries of two-dimensional (2D) magnets have triggered intense research activities to search for atomically thin magnetic systems. Using first-principles calculations, we predict the emergence of 2D magnetism in the monolayers (MLs), few layers, and surfaces of nonmagnetic layered electrides Hf2X (X = S, Se, Te) consisting of three-atom-thick Hf-X-Hf stacks. It is revealed that each bulk Hf2X hosts a novel quantum state of Dirac nodal lines with a high density of states arising from Hf-5d cationic and interlayer anionic electrons around -0.9 eV below the Fermi level EF. However, for the MLs, few layers, and surfaces of Hf2X, such hybridized states are shifted toward EF to generate van Hove singularities, leading to a Stoner instability. The resulting surface ferromagnetism gives rise to strongly spin-polarized topological surface states at Hf2X(001), demonstrating that anionic electrons, 2D magnetism, and band topology are entangled with each other. Our findings will open new perspectives for the discovery of 2D magnets via exploiting surface effects in nonmagnetic layered electrides.
Sferamundi. Prima Parte. Trascrizione dei capitoli I e II
Creators: name: Trujillo, Stefania
Publisher: name: Historias Fingidas
Year: 1970

description: Trascrizione dei capitoli I e II della prima parte di Sferamundi (1558) romanzo che Mambrino Roseo da Fabriano compone come prima continuazione italiana al ciclo spagnolo di Amadís de Gaula. La trascrizione si basa sull’esemplare della Biblioteca Civica di Verona appartenente all’edizione veneziana degli eredi Tramezzino del 1584. Transcription of Chapters I and II of the first part of Sferamundi (1558), the novel that Mambrino Roseo da Fabriano composed as first Italian continuation to the Spanish cycle of Amadís de Gaula. The transcription is based on the copy held by Biblioteca Civica di Verona of the 1584 Venetian edition by heirs Tramezzino.
description: Historias Fingidas, No. 1 (2013)
title: Cats are liquids: Equipercentile equating of different instruments
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2021
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: Equipercentile equating is an alternative version of observed score equating that can accommodate non-normal response distributions. It corrects for differences in mean and standard deviation but also higher distribution moments, such as skewness and kurtosis. This helps harmonize instruments, where, for example, respondents mostly choose high (or low) response options.
description: "Equipercentile equating" ist eine Variante von "observed score equating" die auch nicht normalverteilte Antworten harmonisieren kann. Hierbei werden Unterschiede im Mittelwert, der Standardabweichung, aber auch Unterschiede höherer Verteilungsmomente wie Schiefe und Kurtosis bereinigt. Das hilft zum Beispiel beim Harmonisieren von Instrumenten, bei denen Befragte meist hohe (oder niedrige) Antwortoptionen wählen.
description: GESIS Blog
Sonnenfleckenzeichnung Nr. 3782.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.10.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 2005 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Zusätzlich wurden ergänzende Angaben aufgrund weiterer auswärtiger Beobachtungen direkt auf der Fleckenzeichnung hinzugefügt. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
Sonnenfleckenzeichnung Nr. 3774.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.09.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 1997 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
Capnia coyote Nelson & Baumann 1987
Creators: name: Stewart, Kenneth W.
name: Drake, Eugene F.
name: Stark, Bill P.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Capniidae
Capnia
Capnia coyote

description: Capnia coyote Nelson & Baumann 1987
(Figs. 1, 2, 4, 8, 26-31)
Distribution. California.
Material examined. California: San Bernadino Co., Lake Silverwood, Miller Campground, N 34 ° 16.241 ’ W 17 ° 17.490 ’, 7-III-2007, E.F. Drake, 4♂, 3♀, 1 reared ♂ with exuvium, 15♀ larvae, 1♂ exuvium, 1 confirmed ♀ (by clearing pharate larva), 1 pharate ♀ larva; water temperatrure on collection date 11.11 ° C, air temperature 20 ° C, elevation 1109m, overstory of stream was Jeffrey Pine, Alder, Big Cone Spruce. Willows along stream had been cut for fire prevention. Same locality, 1-II-2011, E.F. Drake, 62♂, 31♀, 1 pair in-copulo.
Characters. Body length ♂ 6.8-7.0mm, ♀ 7.5-9mm. Light to medium brown dorsally, ventrum lighter, little pattern except underlying muscles or developing adult pigment. Antennal segments 44-46, head capsule width ♂ 0.75-0.81mm, ♀ 0.90-1.02mm. Lacinia triangular, palmate, with longitudinally striate palm surface, broad apical teeth, ventral comb of 10-14 bristles and dorsal comb of 16-18 longer bristles (similar to C. ventura, Figs. 50, 51). Right mandible with apical teeth, molar pad of dense stiff bristles, and inner band of hairs from base of apical teeth to molar pad (similar to C. umpqua, Figs. 47, 48). Pronotum with scattered setae over surface, and as a marginal fringe (Fig. 1). Mesosternal Y-arms with enclosed subtriangular area about 0.3 times the intercostal width. Hind wingpads shallowly notched along inner margin (like C. inyo and C. umpqua, Figs. 15, 20); inside forewingpad length ♂ 0.96mm, ♀ 1.26mm. Femora with scattered surface bristles, and tibia with a silky outer fringe (Fig. 2). Abdominal segments with long surface hairs (Figs. 26-29). Sexual dimorphism evident. Male with posterior extension of 10 th tergum, triangular in dorsal view with length 0.52-0.57mm; underlying developing wide-based epiproct visible in pharate individuals (Fig. 4); 10 th tergum in lateral view subtriangular, nearly straight with slightly upturned tip dorsally (Fig. 8). Female without posterior extension of 10 th tergum (Figs. 7, 28). Cercal segments 30-32; cercomeres with apical circlet of short and long bristles, longer dorsal and ventral bristle in lateral view, and occasional fine intercalary hair (Figs. 30-31), not usually visible under 50X light microscopy, and not present in any of the other 4 species studied.
description: Published as part of Stewart, Kenneth W., Drake, Eugene F. & Stark, Bill P., 2011, Larvae Of Five Species Of The Winter Stonefly Genus Capnia (Plecoptera: Capniidae) From California, U. S. A., pp. 167-181 in Illiesia 7 (18) on page 170, DOI: 10.5281/zenodo.4760235
Identification of new hot subdwarf binary systems by means of Virtual Observatory tools
Creators: name: Solano, E.
name: Ulla, A.
name: Pérez-Fernández, E.
name: Rodrigo, C.
name: Oreiro, R.
name: Aller, A.
name: Manteiga, M.
name: Santoveña-Gómez, R.
name: Álvarez, M. A.
name: Dafonte, C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The estimation of the binary fraction of hot subdwarfs is key to shed light on the different evolution scenarios proposed to explain the loss of the hydrogen envelope during the red giant branch phase. In this paper we analyse the spectral energy distribution of the hot subdwarfs included in a recent and comprehensive catalogue with the aim of identifying companions. Our methodology shows a performance superior to the photometric criteria used in that study, identifying 202 objects wrongly classified as binaries according to their spectral energy distributions, and finding 269 new binaries. Out of an initial sample of 3186 objects, we classified 2469 as single and 615 as binary hot subdwarfs. The rest of the objects (102) were not classified because of their inadequate spectral energy distribution fitting due, in turn, to poor quality photometry. Effective temperatures, luminosities and radii were computed for 192 singles and 42 binaries. They, in particular the binary sample, constitute an excellent dataset to further perform a more careful spectroscopic analysis that could provide detailed values for the chemical composition, masses, ages, rotation properties or reflection effects for the shortest-period systems. The results obtained in this paper will be used as a reference for a forthcoming work where we aim to generalize binary and single hot subdwarf classification using Artificial Intelligence-based techniques.
description: 8 pages, 8 figures
Additional file 1 of Survival prediction models: an introduction to discrete-time modeling
Creators: name: Suresh, Krithika
name: Severn, Cameron
name: Ghosh, Debashis
Publisher: name: figshare
Year: 2022
Subjects: subject: Statistics
subject: FOS: Mathematics
subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Additional file 1 Supplementary Material.
Sonnenfleckenzeichnung Nr. 3657.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 30.05.1951, erstellt als Beobachtung im Projektionsverfahren Nr. 1883 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1951

description: Bleistiftzeichnung mit Tinte und Farbstift, erstellt für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Merz-Refraktor mit 13.5 cm Öffnung und 195 cm Brennweite, vereinzelt andere Instrumente wie Tel. 88x; Sonnenbild D = 25 cm. - Auf der Zeichnung wird zum Teil das Instrument vermerkt bzw. die Zählung der Beobachtungen im Projektionsverfahren fortgesetzt. Sporadisch sind Resultate mehrerer Aufnahmen pro Tag aufgelistet. Zuhanden der späteren statistischen Verarbeitung sind die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Zeichnung aus der Zeit der Beobachtertätigkeit von Ing. Karl Rapp als Privat-Astronom, die er seit den Neunzehnvierziger Jahren für die Eidgenössische Sternwarte Zürich ausführte. Aus den ersten zwei Jahren der freiwilligen Mitarbeit sind nur einzelne Stücke überliefert. Erst zwei Jahre später ist jeweils eine ergänzende Serie in Zürich aufbewahrt worden. Nochmals fünf Jahre später arbeitete Karl Rapp neu auf vertraglicher Basis weiter mit, bis schliesslich nach einem weiteren Jahrzehnt die permanente Beobachtungsstation in Locarno-Monti geschaffen wurde, welche an die langjährige Serie von Karl Rapp anknüpfte
title: (Not) by any stretch of the imagination: A cautionary tale about linear stretching
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2021
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: Linear stretching is a frequently used approach to combine data from response scales with different numbers of response options. In linear stretching, the scales’ minimum and maximum scores are set as equal, respectively, and all values in between are spread with equal distances within this range. However, while temptingly easy to use, linear stretching runs the risk of seriously biasing analyses in the harmonized dataset.
description: Linear stretching ist ein häufig verwendeter Ansatz, um Daten von Antwortskalen mit unterschiedlich vielen Antwortoptionen zu kombinieren. Bei linear stretching werden die jeweils die kleinsten und größten möglichen Antwortoptionen gleichgesetzt und alle Antwortoptionen dazwischen mit gleichen Abständen gestreckt. Der Ansatz ist verlockend einfach anzuwenden, aber birgt die Gefahr Analysen mit dem harmonisierten Datensatz ernsthaft zu verzerren.
description: GESIS Blog
The Nitrogen Content in the Fruiting Body and Mycelium of Pleurotus Ostreatus and Its Utilization as a Medium Component in Thraustochytrid Fermentation
Creators: name: Schütte, Lina
name: Hausmann, Katharina
name: Schwarz, Christoph
name: Ersoy, Franziska
name: Berger, Ralf G.
Publisher: name: Basel : MDPI
Year: 2024
Subjects: subject: Basidiomycota
subject: bioprocess
subject: medium substitution
subject: nitrogen source
subject: spent mycelium side stream
subject: squalene
subject: thraustochytrids
subject: triterpenes
subject: Dewey Decimal Classification::500 | Naturwissenschaften::570 | Biowissenschaften, Biologie

description: Following the idea of a circular bioeconomy, the use of side streams as substitutes for cultivation media (components) in bioprocesses would mean an enormous economic and ecological advantage. Costly compounds in conventional media for the production of the triterpene squalene in thraustochytrids are the main carbon source and complex nitrogen sources. Among other side streams examined, extracts from the spent mycelium of the basidiomycete Pleurotus ostreatus were best-suited to acting as alternative nitrogen sources in cultivation media for thraustochytrids. The total nitrogen (3.76 ± 0.01 and 4.24 ± 0.04%, respectively) and protein (16.47 ± 0.06 and 18.57 ± 0.18%, respectively) contents of the fruiting body and mycelium were determined. The fungal cells were hydrolyzed and extracted to generate accessible nitrogen sources. Under preferred conditions, the extracts from the fruiting body and mycelium contained 73.63 ± 1.19 and 89.93 ± 7.54 mM of free amino groups, respectively. Cultivations of Schizochytrium sp. S31 on a medium using a mycelium extract as a complex nitrogen source showed decelerated growth but a similar squalene yield (123.79 ± 14.11 mg/L after 216 h) compared to a conventional medium (111.29 ± 19.96 mg/L, although improvable by additional complex nitrogen source).
title: Verändern sich Effekte individueller Religiosität auf Einstellungen durch die Säkularisierung?
Creators: name: Siegers, Pascal
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2021
Subjects: subject: Sociology of Religion
subject: Secularization
subject: Comparative Social Research
subject: Prosocial Behavior

description: The Covid-19 pandemic has thrust scientists and science explainers into the public eye. Although we may think of their presence in the media as something new, popularization has in fact been part of science since there has been science. Today’s scientists who go on talk shows, record podcasts, or fight disinformation on Twitter are beholden to their forebears in many ways. This article explores the history of popular science in Germany since the nineteenth century and how it has lead to the present moment in science communication.One might think that with the decline of individual religiosity in the secularization process, the effects of religiosity on attitudes and behavior would also disappear. However, this finding is disputed in research. There is evidence that the effects of individual religiosity actually increase as a result of secularization.
description: Man könnte meinen, mit dem Rückgang individueller Religiosität im Säkularisierungsprozess verschwinden auch die Effekte der Religiosität auf Einstellungen und Verhalten. Dieser Befund ist in der Forschung allerdings umstritten. Denn es gibt Hinweise darauf, dass die Effekte individueller Religiosität in Folge der Säkularisierung sogar zunehmen.
description: GESIS Blog
Wavelike nature of the vertical shear instability in global protoplanetary disks
Creators: name: Svanberg, Eleonora
name: Cui, Can
name: Latter, Henrik N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The vertical shear instability (VSI) is a robust phenomenon in irradiated protoplanetary disks (PPDs). The majority of previous numerical simulations have focused on the turbulent properties of its saturated state. However, the saturation of the VSI manifests as large-scale coherent radially travelling inertial waves. In this paper, we study inertial-wave-disk interactions and their impact on VSI saturation. Inertial-wave linear theory is developed and applied to a representative global 2D simulation using the Athena++ code. It is found that the VSI saturates by separating the disk into several radial wave zones roughly demarcated by corotation resonances (turning points); this structure also manifests in modest radial variations in the vertical turbulence strength. Future numerical work should employ large radial domains to accommodate this radial structure of the VSI, while concurrently adopting sufficiently fine resolutions to resolve the parametric instability that attacks the saturated VSI inertial waves.
description: 8 pages, 6 figures, accepted for publication in MNRAS
Capnia inyo Nelson & Baumann 1987
Creators: name: Stewart, Kenneth W.
name: Drake, Eugene F.
name: Stark, Bill P.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Capniidae
Capnia
Capnia inyo

description: Capnia inyo Nelson & Baumann 1987
(Figs. 15-19, 32-37)
Distribution. California.
Material examined. California: Inyo Co., Lone Pine Creek, Lone Pine Campground, N 36 ° 35.860 ’ W 118 ° 11.203 ’, Elev. 1795m, 17-18-II-2010, E. F. Drake. 33♂, 14♀, 5 reared ♂ with exuviae, 3 reared ♀ with exuviae, 1 partially emerged ♂ in larval exuviumaedeagus everted, 7♂ larvae, 22♀ larvae, 3♂ exuviae, 1♀ exuvium; water temperature on collection date 3.3 ° C, snow on ground.
Characters. Body length ♂ 6.6-6.8mm, ♀ 6.9-7.2mm. Light to medium brown dorsally, ventrum lighter, little pattern except underlying muscles or developing adult pigment (Fig. 15). Antennal segments 42-44, head capsule width ♂ 0.72-0.75mm, ♀ 0.84-0.0.90mm. Lacinia and mandibles as described for C. umpqua and C. ventura (Figs. 44-48, 50-53). Pronotum with setae scattered over surface and as a sparse marginal fringe (Fig. 15). Mesosternal Y-arms enclose a subtriangular area about 0.3 times the intercostal width (Fig. 16). Hind wingpads shallowly notched along inner margins (Fig. 15); inside forewingpad length ♂ 0.96-0.99mm, ♀ 1.44-1.50mm. Femora bear scattered surface bristles, and tibia with a silky outer fringe (Fig. 15). Abdominal segments with long surface hairs (Figs. 32, 33). Sexual dimorphism evident. Male 10 th tergum with 0.7-0.8mm long tubular posterior extension in dorsal view (Fig. 15); underlying tubular developing epiproct visible in pharate individuals (Fig. 15); 10 th tergum in lateral view tubular and downcurved (Figs. 17, 34). Female without posterior extension of 10 th tergum (Fig. 18). Cercal segments about 32; cercomeres with apical circlet of short and long bristles, longer dorsal and ventral bristle in lateral view, and no evident intercalary hairs (Fig. 35-37).
description: Published as part of Stewart, Kenneth W., Drake, Eugene F. & Stark, Bill P., 2011, Larvae Of Five Species Of The Winter Stonefly Genus Capnia (Plecoptera: Capniidae) From California, U. S. A., pp. 167-181 in Illiesia 7 (18) on page 170, DOI: 10.5281/zenodo.4760235
Sonnenfleckenzeichnung Nr. 15491.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.08.1943, erstellt von William Brunner, Assistent
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1943

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich, später ergänzt mit einer kleinen Tabelle für die Auszählung der Flecken nach ihrer Verteilung auf Abschnitte der sichtbaren Sonnenhälfte, nach Quadrant bzw. nach Halbkugel (N, S, W, E). Instrument: Kern-Merz-Refraktor.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Unter Umständen sind Angaben zu Protuberanzen vermerkt
A simple data-driven method to optimise the penalty strengths of penalised models and its application to non-parametric smoothing
Creators: name: Thomas, Jens
name: Lipka, Mathias
Publisher: name: arXiv
Year: 2022
Subjects: subject: Methodology (stat.ME)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: Information of interest can often only be extracted from data by model fitting. When the functional form of such a model can not be deduced from first principles, one has to make a choice between different possible models. A common approach in such cases is to minimise the information loss in the model by trying to reduce the number of fit variables (or the model flexibility, respectively) as much as possible while still yielding an acceptable fit to the data. Model selection via the Akaike Information Criterion (AIC) provides such an implementation of Occam's razor. We argue that the same principles can be applied to optimise the penalty-strength of a penalised maximum-likelihood model. However, while in typical applications AIC is used to choose from a finite, discrete set of maximum-likelihood models the penalty optimisation requires to select out of a continuum of candidate models and these models violate the maximum-likelihood condition. We derive a generalised information criterion AICp that encompasses this case. It naturally involves the concept of effective free parameters which is very flexible and can be applied to any model, be it linear or non-linear, parametric or non-parametric, and with or without constraint equations on the parameters. We show that the generalised AICp allows an optimisation of any penalty-strength without the need of separate Monte-Carlo simulations. As an example application, we discuss the optimisation of the smoothing in non-parametric models which has many applications in astrophysics, like in dynamical modeling, spectral fitting or gravitational lensing.
description: Accepted for publication in MNRAS, 12 pages, 9 figures
Participation 3.0 in the implementation of the energy transition—Components and effectiveness of an interactive dialogue tool (Vision:En 2040)
Creators: name: Thiele, Julia
name: Wiehe, Julia
name: Haaren, Christina Von
Publisher: name: San Francisco, Calif. : Public Library of Science
Year: 2024
Subjects: subject: Awareness
subject: Behavioral Research
subject: Electricity
subject: Germany
subject: Humans
subject: Physical Phenomena
subject: agricultural worker
subject: attitude
subject: conceptual framework
subject: content analysis
subject: decision making
subject: electric power plant
subject: electricity
subject: empowerment
subject: energy conservation
subject: energy transition
subject: environmental impact
subject: environmental planning
subject: geography
subject: human
subject: interactive dialogue tool (Vision:En 2040)
subject: knowledge
subject: Likert scale
subject: motivation
subject: participation
subject: physical phenomena
subject: procedures, parameters and devices
subject: qualitative research
subject: questionnaire
subject: renewable energy
subject: social interaction
subject: social learning
subject: sociodemographics
subject: wind farm
subject: awareness
subject: behavioral research
subject: Dewey Decimal Classification::500 | Naturwissenschaften
subject: Dewey Decimal Classification::600 | Technik::610 | Medizin, Gesundheit

description: The allocation of renewable energy plants, especially wind turbines, is stagnating in Germany. Although the citizens approve of the energy transition, they resist concrete local projects. In recent years, research has shown that interactive map applications support participatory planning through motivation, social interaction, and knowledge transfer. We aim to reduce biases against renewable energy (RE) and support informed decision making while accepting local responsibility. We hypothesized that finding a new gamified participation format, based on behavioral mechanisms, would strengthen the empowerment of people. To this end, we designed a dialogue tool and participation format,’Vision:En 2040’, which combines: (i) a precise target electricity yield, (ii) an interactive map showing results of people’s actions, information about environmental impacts, and (iii) game rules which foster cooperation. In facilitated workshops, participants simulate the allocation of wind and photovoltaic power plants in their municipality to achieve a target electricity yield. The developed tool is based on methods of environmental planning and geoinformatics.’Vision:En 2040’ was systematically tested with a technical test and a pre-test. In addition, its impact on participants was assessed through surveys and qualitative content analysis. The evaluation results show that the tool can influence the acceptance of the energy transition in terms of attitude. Through’Vision:En 2040’, participants became aware of the community’s responsibility in the energy transition and expanded their knowledge. In addition, decision makers used the workshop results to plan RE sites. Our results indicate that’Vision:En 2040’ is helpful for informal citizen participation in accelerating the energy transition.
First optical identification of the SRG/eROSITA-detected supernova remnant G 116.6-26.1 I. Preliminary results
Creators: name: Palaiologou, E. V.
name: Leonidaki, I.
name: Kopsacheili, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The supernova remnant (SNR) candidate G 116.6-26.1 is one of the few high Galactic latitude ($|b| > 15^o$) remnants detected so far in several wavebands. It was discovered recently in the SRG/eROSITA all-sky X-ray survey and displays also a low-frequency weak radio signature. In this study, we report the first optical detection of G 116.6-26.1 through deep, wide-field and higher resolution narrowband imaging in $\rm Hα$, [S II] and [O III] light. The object exhibits two major and distinct filamentary emission structures in a partial shell-like formation. The optical filaments are found in excellent positional match with available X-ray, radio and UV maps, can be traced over a relatively long angular distance (38' and 70') and appear unaffected by any strong interactions with the ambient interstellar medium. We also present a flux-calibrated, optical emission spectrum from a single location, with Balmer and several forbidden lines detected, indicative of emission from shock excitation in a typical evolved SNR. Confirmation of the most likely SNR nature of G 116.6-26.1 is provided from the observed value of the line ratio $\rm [S\, II] / Hα= 0.56 \pm 0.06$, which exceeds the widely accepted threshold 0.4, and is further strengthened by the positive outcome of several diagnostic tests for shock emission. Our results indicate an approximate shock velocity range $70-100\, km\, s^{-1}$ at the spectroscopically examined filament, which, when combined with the low emissivity in $\rm Hα$ and other emission lines, suggest that G 116.6-26.1 is a SNR at a mature evolutionary stage.
description: Accepted for publication in MNRAS, 15 pages
title: The new normal: Linear equating of different instruments
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2021
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: As an alternative to linear stretching, we look into the observed score equating approach in this post and the next. The easiest form of observed score equating is linear equating: a powerful approach that corrects for biases in the mean and standard deviation while harmonizing different instruments.
description: Als alternative zu "linear stretching" betrachten wir uns dieses und nächstes Mal den "observed score equating"-Ansatz. Die einfachste Variante des "observed score equatings" ist "linear equating": ein mächtiger Ansatz, der Verzerrungen des Mittelwerts und der Standardabweichung bei der Harmonisierung unterschiedlicher Messinstrumente korrigiert.
description: GESIS Blog
title: Human Rights – Erosion of a Human History Milestone?
Creators: name: Repke, Lydia
name: Link, Emma
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Black Lives Matter
subject: Death Penalty
subject: Eurobarometer
subject: EVS
subject: Homosexuality
subject: Women's Rights
subject: Human Rights

description: On 10 December is Human Rights Day. This year, the United Nations has given the day the motto “Recover Better – Stand Up for Human Rights.” Especially now, we need to tackle the shortcomings revealed by the corona crisis to manage our shared future.
description: Am 10. Dezember ist Tag der Menschenrechte. In diesem Jahr haben die Vereinten Nationen dem Tag das Motto „Recover Better – Stand Up for Human Rights“ gegeben. Besonders jetzt müssen wir uns mit den durch die Corona-Krise offengelegten Versäumnissen befassen, um unsere gemeinsame Zukunft meistern zu können.
description: GESIS Blog