cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Radiative shock oscillation model for the long-term flares of Sgr A*
Creators: name: Okuda, T.
name: Singh, C. B.
name: Aktar, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We examine time-dependent 2D relativistic radiation MHD flows to develop the shock oscillation model for the long-term flares of Sgr A*. Adopting modified flow parameters in addition to the previous studies, we confirm quasi-periodic flares with periods of $\sim$ 5 and 10 days which are compatible with observations by Chandra, Swift, and XMM-Newton monitoring of Sgr A*. Using a simplified two-temperature model of ions and electrons, we find that the flare due to synchrotron emission lags that of bremsstrahlung emission by 1 -- 2 hours which are qualitatively comparable to the time-lags of 1 -- 5 hours reported in several simultaneous observations of radio and X-ray variability in Sgr A*. The synchrotron emission is confined in a core region of 3 $R_{\rm g}$ size with the strong magnetic field, while the bremsstrahlung emission mainly originates in a distant region of 10 -- 20 $R_{\rm g}$ behind the oscillating shock, where $R_{\rm g}$ is the Schwarzschild radius. The time lag is estimated as the transit time of the acoustic wave between the above two regions. The time-averaged distribution of radiation shows a strong anisotropic nature along the rotational axis but isotropic distribution in the radial direction. A high-velocity jet with $\sim 0.6c$ along the rotational axis is intermittently found in a narrow funnel region with a collimation angle $\sim 15^\circ$. The shock oscillating model explains well the flaring rate and the time lag between radio and X-ray emissions for the long-term flares of Sgr A*.
description: 13 pages, 17 figures, accepted to MNRAS
title: International Day of Peace – United in Times of Crisis?
Creators: name: Repke, Lydia
name: Dölken, Johanna
name: Link, Emma
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Peace
subject: Covid-19
subject: Pandemic
subject: Corona
subject: GESIS Panel
subject: Germany

description: The United Nations declared September 21st "International Day of Peace." This year the specified topic is "Shaping Peace Together," and it is concerned with the united fight against Covid-19. To look at what Germany does to fight this battle, we draw upon the data of a special survey on the impact of Covid-19 conducted by the GESIS Panel in March 2020.
description: Die Vereinten Nationen haben den 21. September als Internationalen Tag des Friedens bestimmt. Dieses Jahr findet er unter dem Motto „Shaping Peace Together“ statt und befasst sich mit dem gemeinsamen Kampf gegen Covid-19. Um uns vor Augen zu führen, was Deutschland zu diesem Kampf beiträgt, werfen wir einen Blick auf die Daten einer besonderen Befragung des GESIS Panels zu den Auswirkungen von Covid-19 im März 2020.
description: GESIS Blog
Additional file 1 of Two-dimensional nanovermiculite and polycaprolactone electrospun fibers composite scaffolds promoting diabetic wound healing
Creators: name: Huang, Xingtai
name: Wang, Qirui
name: Mao, Runyi
name: Wang, Zeying
name: Shen, Steve G.F.
name: Mou, Juan
name: Dai, Jiewen
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: Additional file 1: Table S1. Mean diameter size and tensile modulus of PCL/VMT composite scaffolds. Table S2. Released ion concentration of Si and Mg in cell culture medium after incubation for 2 days in the presence of PCL/5%VMT scaffolds. Table S3. Quantitative Real-time PCR primer sequences. Table S4. Antibodies used for Western blot or Immunofluorescence. Figure S1. SEM images of the PCL, PCL/2.5%VMT, PCL/5%VMT, and PCL/10%VMT fibrous composite scaffolds. Figure S2. XRD patterns of PCL, PCL/VMT, and VMT NSs. Figure S3. Size distributions of the PCL, PCL/2.5%VMT, PCL/5%VMT, and PCL/10%VMT fibrous composite scaffolds.Figure S4. (A) Stress-strain curves and (B) tensile modulus ofthe PCL, PCL/2.5%VMT, PCL/5% VMT, and PCL/10%VMT composite scaffolds. Figure S5.(A) SEM images and (B) corresponding size distributions of the PCL, PCL/2.5%VMT, PCL/5%VMT, and PCL/10%VMT composite scaffolds immersed in PBS solutions for 14 days. Figure S6. In vitro hemolysis assay of the PCL, PCL/2.5%VMT, PCL/5%VMT, and PCL/10%VMT composite scaffolds. (A) Photographs and (B) absorbance of supernatants of RBCs exposed to different samples. Figure S7. Effects of PCL/VMT composite scaffolds on NO production in MAECs. (A) Representative fluorescent images of intracellular NO production detected by using DAF-FM probe after incubation for 72 h. (B) The amount of NO released into cell medium from MAECs cultured on the different composite scaffolds after incubation for 72 h using Griess reaction assay kits. Figure S8. Effects of PCL/VMT composite scaffolds on the expression of inflammatory factors in RAW 264.7. Relative mRNA expression of iNOS and Arg in the RAW 264.7 treated with PCL, PCL/2.5%VMT, PCL/5%VMT, PCL/10%VMT without (A) and with (B) LPS.
The Si+SO$_2$ collision and an extended network of neutral-neutral reactions between silicon and sulphur bearing species
Creators: name: Campanha, Danilo R.
name: Mendoza, Edgar
name: Silva, Mateus X.
name: Velloso, Paulo F. G.
name: Carvajal, Miguel
name: Wakelam, Valentine
name: Galvão, Breno R. L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Si+SO$_2$ reaction is investigated to verify its impact on the abundances of molecules with astrochemical interest, such as SiS, SiO, SO and others. According to our results Si($^3$P) and SO$_2$ react barrierlessly yielding only the monoxides SO and SiO as products. No favourable pathway has been found leading to other products, and this reaction should not contribute to SiS abundance. Furthermore, it is predicted that SiS is stable in collisions with O$_2$, and that S($^3$P)+SiO$_2$ and O($^3$P)+OSiS will also produce SO+SiO. Using these results and gathering further experimental and computational data from the literature, we provide an extended network of neutral-neutral reactions involving Si- and S-bearing molecules. The effects of these reactions were examined in a protostellar shock model, using the Nautilus gas-grain code. This consisted in simulating the physicochemical conditions of a shocked gas evolving from $i.$ primeval cold core, $ii.$ the shock region itself, $iii.$ and finally the gas bulk conditions after the passage of the shock. Emphasising on the cloud ages and including systematically these chemical reactions, we found that [SiS/H$_2$] can be of the order of $\sim$ 10$^{-8}$ in shocks that evolves from clouds of $t=1\times 10^6$ yr, whose values are mostly affected by the SiS+O $\longrightarrow$SiO+S reaction. Perspectives on further models along with observations are discussed in the context of sources harbouring molecular outflows.
description: 10 pages, 7 figures. Accepted for publication in Monthly Notices of the Royal Astronomical Society Main Journal
EOS-ESTM: A flexible climate model for habitable exoplanets
Creators: name: Biasiotti, L.
name: Simonetti, P.
name: Vladilo, G.
name: Silva, L.
name: Murante, G.
name: Ivanovski, S.
name: Maris, M.
name: Monai, S.
name: Bisesi, E.
name: von Hardenberg, J.
name: Provenzale, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Rocky planets with temperate conditions provide the best chance for discovering habitable worlds and life outside the Solar System. In the last decades, new instrumental facilities and large observational campaigns have been driven by the quest for habitable worlds. Climate models aimed at studying the habitability of rocky planets are essential tools to pay off these technological and observational endeavours. In this context, we present EOS-ESTM, a fast and flexible model aimed at exploring the impact on habitability of multiple climate factors, including those unconstrained by observations. EOS-ESTM is built on ESTM, a seasonal-latitudinal energy balance model featuring an advanced treatment of the meridional and vertical transport. The novel features of EOS-ESTM include: (1) parameterizations for simulating the climate impact of oceans, land, ice, and clouds as a function of temperature and stellar zenith distance; (2) a procedure (EOS) for calculating the radiative transfer in atmospheres with terrestrial and non-terrestrial compositions illuminated by solar- and non-solar-type stars. By feeding EOS-ESTM with Earth's stellar, orbital and planetary parameters we derive a reference model that satisfies a large number of observational constraints of the Earth's climate system. Validation tests of non-terrestrial conditions yield predictions that are in line with comparable results obtained with a hierarchy of climate models. The application of EOS-ESTM to planetary atmospheres in maximum greenhouse conditions demonstrates the possibility of tracking the snowball transition at the outer edge of the HZ for a variety of planetary parameters, paving the road for multi-parametric studies of the HZ.
description: 22 pages, 14 figures, 10 tables, accepted for publication in MNRAS
มาตรการทางกฎหมายในการคุ้มครองเงินฝาก และเงินค่าหุ้นของสมาชิกสหกรณ์การเงินในประเทศไทย
Creators: name: นุรัตน์ ปวนคำมา, ฤทธิภัฏ กัลยาณภัทรศิษฏ์ และรุ่ง ศรีสมวงษ์
Publisher: name: Mae Fah Luang University
Year: 2017
Subjects: กฎหมายคุ้มครองเงินฝาก / สหกรณ์การเงิน / สหกรณ์ออมทรัพย์ / สหกรณ์เครดิตยูเนียน

description: MFU Connexion: Journal of Humanities and Social Sciences, 6, 2
Stellar migration in the Auriga simulations
Creators: name: Okalidis, Periklis
name: Grand, Robert J. J.
name: Yates, Robert M.
name: Springel, Volker
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the presence and importance of stellar migration in the evolution of 17 Milky-Way like disk galaxies with stellar mass $10 < \textrm{log}(M_{*}/{\rm M}_\odot) < 11$ from the Auriga suite of zoom-in cosmological hydrodynamical simulations. We compare the birth radii of the stars to their radii at $z=0$ for each system and present mean values of the strength of stellar migration as a function of radius and stellar age which vary between 1-4 kpc. We also investigate the effect of migration on age and metallicity radial profiles in the disks. We find several cases of age gradient flattening due to migration, but significant changes to metallicity profiles only for older stellar populations and disks that develop a strong bar. Furthermore, we study stellar migration from the perspective of the change of the galactocentric radius ($ΔR$) and orbital guiding centre radius ($ΔR_g$) of stellar particles between given time intervals. We find that stars migrate approximately as a diffusion process only in the outer parts of the disks and for particular galaxies that have a weak bar. Strongly barred galaxies in our sample show larger stellar migration but its timestep evolution is slower-than-diffusion. Finally, we give parametrisations that encapsulate the dependence of the strength of the radial migration as a function of time and radius, for incorporation into (semi-)analytic models of galaxy evolution.
description: 21 pages, 19 figures, Accepted for publication in MNRAS
Bases folklóricas y culturales en las relaciones amorosas entre moros y cristianos en el Palmerín de Olivia (libros I y II)
Creators: name: Bueno Serrano, Ana Carmen
Publisher: name: Historias Fingidas
Year: 1970

description: Durante siglos, la convivencia entre moros y cristianos ha generado abundante literatura. En este trabajo se da una vuelta de tuerca más al tema tomando como referencia dos episodios amorosos del Palmerín de Olivia en los que el amor como cautiverio y como herida. En ambos las relaciones afectivas entre los credos son desiguales porque son esporádicas y encaminadas a perfilar las virtudes o defectos del caballero. Se recurre a las constantes de la literatura de la época, haciendo caso omiso de los problemas (y soluciones) del momento, que se eluden imprimiendo a los textos un pensamiento patriarcal y católico. During centuries, Muslims and Christians coexistence has generated a huge amount of literature. This works tries to give a turn to the subject taking as a reference two amatory episodes of the Palmerín of Olivia in which love is represented as captivity and wound. In both, the affective relations between the creeds are irregular because they are sporadic and directed to outline the virtues or defects of the knight. The novel refers to the literary tradition of the period and doesn’t take in consideration the problems (and solutions) of the contemporary age.
description: Historias Fingidas, No. 1 (2013)
Stichi k Sonečke
Creators: name: Cvetaeva, Marina
Publisher: name: [s.n.]
Year: 1938

description: Korrekturabzug
description: Erschienen in: Russkije zapiski 1938, Nr. 3, S. 166-171
description: Marina Cvetaeva
description: Russisch
description: Verzeichnung=Description=Inventaire November 2018 HAN-Katalogisierungsregeln
Statistics of BY Draconis Chromospheric Variable Stars
Creators: name: Chahal, Deepak
name: de Grijs, Richard
name: Kamath, Devika
name: Chen, Xiaodian
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present an extensive catalogue of BY Draconis (BY Dra)-type variables and their stellar parameters. BY Dra are main-sequence FGKM-type stars. They exhibit inhomogeneous starspots and bright faculae in their photospheres. These features are caused by stellar magnetic fields, which are carried along with the stellar disc through rotation and which produce gradual modulations in their light curves (LCs). Our main objective is to characterise the properties of BY Dra variables over a wide range of stellar masses, temperatures and rotation periods. A recent study categorised 84,697 BY Dra variables from Data Release 2 of the Zwicky Transient Facility based on their LCs. We have collected additional photometric data from multiple surveys and performed broad-band spectral energy distribution fits to estimate stellar parameters. We found that more than half of our sample objects are of K spectral type, covering an extensive range of stellar parameters in the low-mass regime (0.1-1.3 M$_{\odot}$ ). Compared with previous studies, most of the sources in our catalogue are rapid rotators, and so most of them must be young stars for which a spin-down has not yet occurred. We subdivided our catalogue based on convection zone depth and found that the photospheric activity index, $S_{\rm ph}$, is lower for higher effective temperatures, i.e., for thinner convective envelopes. We observe a broad range of photospheric magnetic activity for different spectral classes owing to the presence of stellar populations of different ages. We found a higher magnetically active fraction for K- than M-type stars.
description: 12 pages, 13 figures
Povĕst' o Sonečkě
Creators: name: Cvetaeva, Marina
Publisher: name: [s.n.]
Year: 1938

description: In: Russkije zapiski 1938, Nr. 3, S. 36-103; mit handschr. Korrekturen und einer handschriftlichen Anmerkung von Marina Cvetaeva am Schluss des Textes.
description: Marina Cvetaeva
description: Russisch
description: Verzeichnung=Description=Inventaire November 2018 HAN-Katalogisierungsregeln
Additional file 1 of Behavioral manifestations in rodent models of autism spectrum disorder: protocol for a systematic review and network meta-analysis
Creators: name: Panzenhagen, Alana Castro
name: Cavalcanti, Amanda
name: Stein, Dirson João
name: de Castro, Ligia Lins
name: Vasconcelos, Mailton
name: Abreu, Mariana Boechat
name: Almeida, Roberto Farina
name: Bertoglio, Leandro José
name: Herrmann, Ana Paula
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. Search strategy. The complete search strategy syntax for PubMed, Web of Science, and Scopus databases.
title: Adventures in ex-post harmonization: Frankenstein’s Creature
Creators: name: Singh, Ranjit K.
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Ex-Post Harmonization Adventures
subject: Comparability
subject: Survey Methodology
subject: FAIR Data Principles
subject: Open Data

description: In this series of blog posts, we will explore ex-post harmonization: the art of combining data from different surveys. In this introductory post, I explain the motivation behind the series and outline the upcoming topics. The series is aimed at both seasoned ex-post harmonization practitioners as well as researchers who are curious about ex-post harmonization and how it can enrich their research projects.
description: Dies ist der Auftakt einer Reihe an Blogposts über ex-post Harmonisierung: der Kunst Daten aus verschiedenen Umfragen zu kombinieren. In diesem Intro geht es um die Motivation hinter der Serie und um die kommenden Themen. Die Serie richtet sich sowohl an erfahrene ex-post Harmonisierungspraktiker*innen, als auch an Forschende, die neugierig darauf sind, wie ex-post Harmonisierung ihre Forschungsprojekte bereichern kann.
description: GESIS Blog
Interacting planetary nebulae III: Verification and galactic population based on the measurements of Gaia EDR3
Creators: name: Mohery, M.
name: Ali, A.
name: Mindil, A.
name: Alghamdi, S. 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: The phenomenon of interaction between planetary nebulae (PNe) and the interstellar medium (ISM) is one of the significant issues in the field of astrophysics. The main objective of this paper is to verify the interaction process for objects that have been known as interacting PNe (IPNe) in the literature. This study is based on parallax and proper motion observations facilitated recently by the early third data release of the Gaia space mission. Based on the proper nebular central star (CS) motion towards the region of interaction between the PN and ISM, we were able to verify the interaction process for a group of 68 PNe and disprove the interaction process for a group of 33 PNe. The members of both groups were confirmed as genuine PN-ISM interacting objects in the literature. The members belonging to the 33 PNe group are false PN-ISM interacting objects that mimic the structure of IPNe. Moreover, we calculated the physical and kinematic properties of the verified group and analyzed their galactic population classification using reliable and precise measurements of the proper motion and parallax of the CS. We find that 41\% and 41\% of this group are associated with galactic thin and thick disks, respectively, while 18\% are members of thin or thick disks. The kinematical results show that the galactic thin-disk members have smaller vertical galactic heights, space velocities, and peculiar velocities than those belonging to the galactic thick disk.
description: 18 pages, 7 figures, 5 tables
АНАЛИЗ ПРОЦЕССА ВЫРАБОТКИ ЭЛЕКТРОЭНЕРГИИ С ПОМОЩЬЮ СОЛНЕЧНЫХ БАТАРЕЙ
Creators: name: Алламуратов, Т.К.
name: Абдуллаева, Д.К.
Publisher: name: Zenodo
Year: 2024

description: В заключении мы дадим рекомендации по использованию технологию мониторинга на основе IoT для повышения эффективности выработки электроэнергии. Применение таких технологий позволит осуществлять постоянный контроль и оптимизацию работы солнечных панелей, что значительно повысит их производительность и надежность. Эти меры способствуют не только увеличению эффективности использования солнечной энергии, но и созданию более устойчивой и управляемой энергосистемы.
Sonnenfleckenzeichnung Nr. 119.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.05.1968, erstellt von Araldo Pittini, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1968

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
Capnia undefined-1
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 undefined-1

description: Provisional Key to Mature Male Larvae of Five California Capnia Species
1 Tergum 10 with 0.7-0.8 mm tubular posterior extension; developing tubular epiproct visible in pharate individuals (Figs. 15, 17, 34) ………… inyo
1’ Tergum 10 shorter than 0.5 mm, its posterior extension variably shaped (Figs. 4, 5, 6, 8, 10, 11, 12, 40, 55) ………………………………………….. 2
2 Posterior extension of 10 th tergum subtriangular in dorsal view, with wide-based developing epiproct visible in pharate individuals (Fig. 4); dorsal margin nearly straight in lateral view, with slightly upturned tip (Fig. 8) ……………… coyote
2’ Posterior extension of 10 th tergum with dorsal margin sharply upturned in lateral view (Figs. 5, 6, 40), or evenly downturned (Figs. 54-55), or nearly straight with slightly downturned tip (Fig. 10); developing epiproct in pharate individuals variously shaped (Figs. 5, 10, 12) ……………… 3
3 Base of tergum 10 extension with cross-striated surface, and in lateral view, with evenly downturned dorsal margin (Figs. 54-55) ... ventura
3’ Base of tergum 10 with smooth, unstriated surface ……………………………………………………… 4
4 Tergum 10 extension sharply upturned in lateral view (Figs. 5, 6, 40) ………………………….. teresa
4’ Tergum 10 extension with dorsal margin nearly straight, but with slightly downturned tip in lateral view ……………………………….. umpqua
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 178, DOI: 10.5281/zenodo.4760235
Oxygen and calcium nebular emission line relationships in core-collapse supernovae and Ca-rich transients
Creators: name: Prentice, Simon
name: Maguire, Kate
name: Siebenaler, Louis
name: Jerkstrand, Anders
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: This work examines the relationships between the properties (flux ratios, full width at half-maximum velocities) of the [O I] $λλ$6300, 6364, [Ca II] $λλ$7291, 7323, and the Ca II near-infrared triplet, emission lines of a large sample of core-collapse supernovae (SNe) and Ca-rich transients (509 spectra of 86 transients, of which 10 transients are Ca-rich events). Line-flux ratios as a function of time were investigated with differences identified between the transient classes, in particular the Type II SNe were found to have distinct line-flux ratios compared to stripped-envelope (SE) SNe. No correlation was found between the [Ca II]/[O I] flux ratios of SE-SNe and their ejecta masses and kinetic energies (as measured from light curve modelling), suggesting that there may be a contribution from an additional power source in more luminous SE-SNe. We found that the mean characteristic width of the [Ca II] emission line is less than the [O I] emission line for all SN types, indicating that the [Ca II] emission typically originates from deeper in the ejecta than [O I]. This is in some tension with standard models for emission in Type II SNe. The emission line properties of Type II SNe were also compared to theoretical models and found to favour lower mass tracks ($M_\mathrm{ZAMS}$ $<$ 15 M$_{\odot}$), with no evidence found for significant mixing of $^{56}$Ni into the H envelope nor Ca mixed into the O shell. The flux ratios of some superluminous SNe were found to be similar to those of SE-SNe when scaling to account for their longer rise times was applied (although we caution the sample size is small).
description: 21 pages, 12 figures, accepted for publication in MNRAS
Additional file 2 of Behavioral manifestations in rodent models of autism spectrum disorder: protocol for a systematic review and network meta-analysis
Creators: name: Panzenhagen, Alana Castro
name: Cavalcanti, Amanda
name: Stein, Dirson João
name: de Castro, Ligia Lins
name: Vasconcelos, Mailton
name: Abreu, Mariana Boechat
name: Almeida, Roberto Farina
name: Bertoglio, Leandro José
name: Herrmann, Ana Paula
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 2. Behavioral outcomes. List of behavioral categories and examples of experimental paradigms.
Relic jet activity in "Hanny's Voorwerp" revealed by the LOFAR Two metre Sky Survey
Creators: name: Smith, D. J. B.
name: Krause, M. G.
name: Hardcastle, M. J.
name: Drake, A. B.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report new observations of "Hanny's Voorwerp" (hereafter HV) taken from the second data release of the LOFAR Two-metre Sky Survey (LoTSS). HV is a highly-ionised region in the environs of the galaxy IC2497, first discovered by the Galaxy Zoo project. The new 150MHz observations are considered in the context of existing multi-frequency radio data and archival narrow-band imaging from the Hubble Space Telescope, centred on the [Oiii] emission line. The combined sensitivity and spatial resolution of the LoTSS data -- which far exceed what was previously available at radio frequencies -- reveal clear evidence for large-scale extended emission emanating from the nucleus of IC2497. The radio jet appears to have punched a hole in the neutral gas halo, in a region co-located with HV. The new 150MHz data, alongside newly-processed archival 1.64GHz eVLA data, reveal that the extended emission has a steep spectrum, implying an age $>10^8$yr. The jet supplying the extended 150MHz structure must have "turned off" long before the change in X-ray luminosity reported in recent works. In this picture, a combination of jet activity and the influence of the radiatively efficient active galactic nucleus are responsible for the unusual appearance of HV.
description: 7 pages, 4 figures, accepted for publication in MNRAS
On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
Creators: name: Jones, G. T.
name: Stanway, E. R.
name: Carnall, A. C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The physical properties of galaxies are encoded within their spectral energy distribution and require comparison with models to be extracted. These models must contain a synthetic stellar population and, where infrared data is to be used, also consider prescriptions for energy reprocessing and re-emission by dust. While many such models have been constructed, there are few analyses of the impact of stellar population model choice on derived dust parameters, or vice versa. Here we apply a simple framework to compare the impact of these choices, combining three commonly-used stellar population synthesis models and three dust emission models. We compare fits to the ultraviolet to far-infrared spectral energy distributions of a validation sample of infrared-luminous galaxies. We find that including different physics, such as binary stellar evolution, in the stellar synthesis model can introduce biases and uncertainties in the derived parameters of the dust and stellar emission models, largely due to differences in the far-ultraviolet emission available for reprocessing. This may help to reconcile the discrepancy between the cosmic star formation rate and stellar mass density histories. Notably the inclusion of a dusty stellar birth cloud component in the dust emission model provides more flexibility in accommodating the stellar population model, as its reemission is highly sensitive to the ultraviolet radiation field spectrum and density. Binary populations favour a longer birth cloud dissipation timescale than is found when assuming only single star population synthesis.
description: 16 Pages, 9 Figures + appendix, accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 15481.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 09.08.1943, erstellt von William Otto Brunner
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
Sonnenfleckenzeichnung Nr. 15480.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 08.08.1943, 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
Savarna Huber 2005
Creators: name: Lan, Tianqi
name: Yao, Zhiyuan
name: Zheng, Guo
name: Wongprom, Prasit
name: Li, Shuqiang
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Pholcidae
Savarna

description: Genus Savarna Huber, 2005
Savarna Huber 2005: 76. Type species: Savarna thaleban Huber, 2005
The five new species below share all the diagnostic features of Savana: long male palpal trochanter apophysis uniquely attached to femur, male chelicerae with only proximo-lateral apophyses (unmodified), and epigynum without pockets (Huber 2005; Huber et al. 2015b).
description: Published as part of Lan, Tianqi, Yao, Zhiyuan, Zheng, Guo, Wongprom, Prasit & Li, Shuqiang, 2020, Five new species of the spider genus Savarna Huber, 2005 (Araneae: Pholcidae) from Thailand, pp. 311-328 in Zootaxa 4778 (2) on page 312, DOI: 10.11646/zootaxa.4778.2.4, http://zenodo.org/record/3856586
Additional file 1 of Analysis of the causal structure of traits involved in sow lactation feed efficiency
Creators: name: Mora, Mónica
name: David, Ingrid
name: Gilbert, Hélène
name: Rosa, Guilherme J. M.
name: Sánchez, Juan Pablo
name: Piles, Miriam
Publisher: name: figshare
Year: 2022
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 1: Table S1. Posterior means of permanent correlations and 95% highest posterior density (HPD95%) intervals among traits based on the multiple trait animal model and on the structural equation model (SEM). Table S2. Posterior means of contemporary group correlations and 95% highest posterior density (HPD95%) intervals among traits based on the multiple trait animal model and on the structural equation model (SEM). Table S3. Posterior means (posterior SD) of correlated response to selection of each trait of the selection objective. Table S4. Posterior means (posterior SD) of correlated response to selection of each trait of the selection objective.
Sonnenfleckenzeichnung Nr. 15497.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.08.1943, 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
Sonnenfleckenzeichnung Nr. 4692.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.09.1954, erstellt als Beobachtung im Projektionsverfahren Nr. 2759 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1954

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
Sonnenfleckenzeichnung Nr. 4776.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.12.1954, erstellt als Beobachtung im Projektionsverfahren Nr. 2842 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1954

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
Sonnenfleckenzeichnung Nr. 15434.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.06.1943, erstellt von William Otto Brunner
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
Sonnenfleckenzeichnung Nr. 4690.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.09.1954, erstellt als Beobachtung im Projektionsverfahren Nr. 2757 von Karl Rapp in Locarno-Monti
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1954

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
Monitoring Observations of SMC X-1's Excursions (MOOSE) I: Program Description and Initial High-State Spectral Results
Creators: name: Dage, Kristen C.
name: Brumback, McKinley
name: Neilsen, Joey
name: Hu, Chin-Ping
name: Altamirano, Diego
name: Bahramian, Arash
name: Charles, Philip A.
name: Clarkson, William I.
name: Haggard, Daryl
name: Hickox, Ryan C.
name: Kennea, Jamie
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: SMC X-1 has exhibited three super-orbital period excursions since the onset of X-ray monitoring beginning with RXTE's launch in 1995. NICER has recently probed a fourth observed excursion beginning in 2021 with our program Monitoring Observations of SMC X-1's Excursions (MOOSE). These sensitive new MOOSE data probe different super-orbital periods and phases within them. Spectral fits to the high-state continuum during April 2021 to January 2022 show that the intrinsic spectral shapes are characterised by a soft (kT~0.19 keV) disc component and a hard (Gamma~0.7) power-law tail. When the 2021-2022 NICER observations, taken during an excursion, are compared to 2016 XMM-Newton observations (outside of an excursion), we find little evidence for intrinsic spectral variability across the high-states, but find evidence for a >3 sigma change in the absorption, although we caution that there may be calibration differences between the two instruments. Thus, over different lengths of super-orbital periods, we see little evidence for intrinsic spectral changes in the high-state. Upcoming studies of the pulse profiles may shed light on the mechanism behind the excursions.
description: accepted to MNRAS
title: Über die Kunst, Phänomene in den Sozialwissenschaften messbar zu machen
Creators: name: Schmidt, Isabelle
name: Lechner, Clemens
name: Bluemke, Matthias
name: Partsch, Melanie
name: Groskurth, Katharina
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Scale Documentation
subject: Quality Criteria
subject: Reliability
subject: Validity
subject: Open Access

description: An important challenge of social science survey research is to define characteristics (phenomena) of individuals or groups of individuals that are not directly observable and to make them measurable. While it is easy to record observable, factual or objective characteristics (e.g. number of children, income) relatively error-free, this is much more complicated with characteristics that are not directly observable. These include personality traits, cultural capital or political trust. Measuring instruments for such characteristics must be constructed and documented with particular care to ensure the quality of their measurement (more precisely: objectivity, validity and reliability). This article explains how to construct and document such measuring instruments and explains why it is important for research and practice to make documentation of measuring instruments as freely accessible as possible ("open access").
description: Eine wichtige Herausforderung der sozialwissenschaftlichen Umfrageforschung besteht darin, nicht direkt beobachtbare Merkmale (Phänomene) von Personen oder Personengruppen zu definieren und messbar zu machen. Während es vergleichsweise einfach ist, beobachtbare, faktische oder objektive Merkmale (z.B. Kinderzahl, Einkommen) relativ fehlerfrei zu erfassen, ist das mit nicht direkt beobachtbaren Merkmalen deutlich komplizierter. Dazu zählen z.B. Persönlichkeitseigenschaften, kulturelles Kapital oder politisches Vertrauen. Messinstrumente für solche Merkmale müssen besonders sorgfältig konstruiert und dokumentiert werden, um die Qualität deren Messung (genauer: die Objektivität, Validität und Reliabilität) sicherzustellen. Dieser Beitrag erklärt, wie man solche Messinstrumente konstruiert und dokumentiert und erläutert, warum es für Forschung und Praxis wichtig ist, Dokumentationen von Messinstrumenten möglichst frei zugänglich zu machen („Open Access“).
description: GESIS Blog
title: International Youth Day – Rebels With a Cause?
Creators: name: Repke, Lydia
name: Dölken, Johanna
Publisher: name: GESIS - Leibniz Institute for the Social Sciences
publisherIdentifier: https://ror.org/018afyw53
Year: 2020
Subjects: subject: Youth
subject: Social Engagement
subject: Activism
subject: Collective Action
subject: Social Movements
subject: European Social Survey

description: August 12th has been declared “International Youth Day” by the United Nations. This year, the focus is on youth engagement in today’s time. But what do young people fight for, and how do they do it? To answer these questions, we take a look at the data of the European Social Survey.
description: Die Vereinten Nationen haben den 12. August als Internationalen Tag der Jugend festgelegt. In diesem Jahr liegt der Fokus auf dem Engagement junger Menschen in der heutigen Zeit. Aber wofür kämpfen junge Leute eigentlich und wie gehen sie die Sache an? Um diese Fragen zu beantworten, werfen wir einen Blick in die Daten des European Social Survey.
description: GESIS Blog
reXcor: A Model of the X-ray Spectrum of Active Galactic Nuclei that Combines Ionized Reflection and a Warm Corona
Creators: name: Xiang, Xin
name: Ballantyne, D. R.
name: Bianchi, S.
name: De Rosa, A.
name: Matt, G.
name: Middei, R.
name: Petrucci, P. -O.
name: Rozanska, A.
name: Ursini, F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The X-ray spectra of active galactic nuclei (AGNs) often exhibit an excess of emission above the primary power-law at energies <~ $2$ keV. Two models for the origin of this `soft excess' are ionized relativistic reflection from the inner accretion disc and Comptonization of thermal emission in a warm corona. Here, we introduce reXcor, a new AGN X-ray ($0.3$-$100$ keV) spectral fitting model that self-consistently combines the effects of both ionized relativistic reflection and the emission from a warm corona. In this model, the accretion energy liberated in the inner disc is distributed between a warm corona, a lamppost X-ray source, and the accretion disc. The emission and ionized reflection spectrum from the inner $400$ $r_g$ of the disc is computed, incorporating the effects of relativistic light-bending and blurring. The resulting spectra predict a variety of soft excess shapes and sizes that depend on the fraction of energy dissipated in the warm corona and lamppost. We illustrate the use of reXcor by fitting to the joint XMM-Newton and NuSTAR observations of the Seyfert 1 galaxies HE 1143-1820 and NGC 4593, and find that both objects require a warm corona contribution to the soft excess. Eight reXcor table models, covering different values of accretion rate, lamppost height and black hole spin, are publicly available through the XSPEC website. Systematic use of reXcor will provide insight into the distribution of energy in AGN accretion flows.
description: 17 pages, 11 figures, accepted by MNRAS. The reXcor table models can be downloaded here: https://github.com/HEASARC/xspec_localmodels/tree/master/reXcor
Additional file 1 of Generation of an mESC model with a human hemophilia B nonsense mutation via CRISPR/Cas9 technology
Creators: name: Ma, Yanchun
name: Sun, Wenwen
name: Zhao, Lidong
name: Yao, Mingze
name: Wu, Changxin
name: Su, Pengfei
name: Yang, Linhua
name: Wang, Gang
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. STR Analysis.