cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Optical and Ultraviolet Spectroscopy of SN 1995N: Evidence for Strong Circumstellar Interaction
Creators: name: Fransson, Claes
name: Chevalier, Roger A.
name: Filippenko, Alexei V.
name: Leibundgut, Bruno
name: Barth, Aaron J.
name: Fesen, Robert A.
name: Kirshner, Robert P.
name: Leonard, Douglas C.
name: Li, Weidong
name: Lundqvist, Peter
name: Sollerman, Jesper
name: Van Dyk, Schuyler D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Optical and ultraviolet observations of the Type IIn supernova 1995N at epochs between 321 and 1799 days after the explosion show three distinct velocity components. The narrow lines come from circumstellar gas and show both low and high ionization. This component has a low filling factor, and is photoionized by X-rays from the shock. The intermediate component, which is dominated by newly processed oxygen, originates in a shell with velocity of 2500-5000 km/s, and most likely comes from the ejecta. The hydrogen- and helium-dominated gas has a low ionization, a high density, and velocities that extend out to ~10,000 km/s. Strong signatures of Ly-alpha-pumped fluorescence lines of Fe II are seen in the near-infrared and ultraviolet. The He/H ratio, ~ 0.3 by number, and the nitrogen overabundance provide strong evidence for CNO burning products. The fluxes of the broad hydrogen and helium lines decrease considerably faster than the oxygen lines. The H-alpha line profile shows strong evolution, with the red wing decreasing faster than the blue. Possible scenarios, involving either a clumpy circumstellar medium, or an aspherical distribution of the surrounding gas, are discussed based on the line profiles and physical conditions. Finally, we propose that Type IIn supernovae have their origin in red supergiants in a superwind phase.
description: 49 pages, 14 figures. Submitted to ApJ
Seladerma luteolum Delucchi 1955
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Seladerma
Seladerma luteolum

description: Seladerma luteolum Delucchi (Pteromalidae)
 Seladerma luteolum Delucchi, 1955a: 49, 53. Holotype m, Germany (NMW [examined]).
 Material. HOLOTYPE m (cr, left antenna, right wings, left protarsus partly, right mid and hind leg beyond coxa, and left metatarsus lacking, right pedicel with ¯agellum glued beside body) labelled`Collect. G. Mayr; p. 440. 72. Or. Ex.. l; Lamp. ¯aviscapis FoÈrster, Type; 31/6 40.; SELADERMA luteolum n. V. Delucchi det.; TYPE [red]’. One slide (sc) labelled`81; SELADERMA [black underlined] luteolum [red underlined] ala m; L. luteolus [sic]5 ¯aviscapis ala [pasted over by former label]’ with right fore wing of holotype.
 Remarks. Delucchi described the female and stated`Type deÂposeÂ au MuseÂum d’Histoire Naturelle de Vienne.’ but did not specify the number of specimens he had. Holotype subsequently remounted from micro-pin by me. It is a specimen from the FoÈrster collection. One female (cp) in the NMW labelled` ThuÈringen, Schmiedekn.’ and provided with Delucchi’s identi®cation label is not considered as part of the type series, since its data were not mentioned by Delucchi.
 Examination of the name-bearing types and a further three females from Germany and Switzerland (ETHZ, MZL, NMW) con®rmed the apparent synonymy of luteolum with Seladerma bicolor Walker as suggested by Graham (1969: 206).
 Status. Junior synonym of Seladerma bicolor Walker syn. n.
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 103, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Atmospheres and Spectra of Strongly Magnetized Neutron Stars
Creators: name: Ho, Wynn C. G.
name: Lai, Dong
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We construct atmosphere models for strongly magnetized neutron stars with surface fields $B\sim 10^{12}-10^{15}$ G and effective temperatures $T_{\rm eff}\sim 10^6-10^7$ K. The atmospheres directly determine the characteristics of thermal emission from isolated neutron stars, including radio pulsars, soft gamma-ray repeaters, and anomalous X-ray pulsars. In our models, the atmosphere is composed of pure hydrogen or helium and is assumed to be fully ionized. The radiative opacities include free-free absorption and scattering by both electrons and ions computed for the two photon polarization modes in the magnetized electron-ion plasma. Since the radiation emerges from deep layers in the atmosphere with $ρ\ga 10^2$ g/cm$^3$, plasma effects can significantly modify the photon opacities by changing the properties of the polarization modes. In the case where the magnetic field and the surface normal are parallel, we solve the full, angle-dependent, coupled radiative transfer equations for both polarization modes. We also construct atmosphere models for general field orientations based on the diffusion approximation of the transport equations and compare the results with models based on full radiative transport. In general, the emergent thermal radiation exhibits significant deviation from blackbody, with harder spectra at high energies. The spectra also show a broad feature ($ΔE/\Ebi\sim 1$) around the ion cyclotron resonance $\Ebi=0.63 (Z/A)(B/10^{14}{G})$ keV, where $Z$ and $A$ are the atomic charge and atomic mass of the ion, respectively; this feature is particularly pronounced when $\Ebi\ga 3k\Teff$. Detection of the resonance feature would provide a direct measurement of the surface magnetic fields on magnetars.
description: 29 pages, 11 figures; corrected factor of 2 in He models: minor changes to figs 4 and 9 as a result; other very minor changes
Torrenticola (Torrenticola) similis
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Torrenticolidae
Torrenticola
Torrenticola similis

description: Torrenticola (Torrenticola) similis (Viets, 1939)
 Atractides elliptica similis Viets, 1939a: 9; E. Angelier 1950a: 85; C. Angelier 1951b: 75.
 Torrenticola similis (Viets, 1939): E. Angelier 1957: 68, 1953b: 91, 1957a: 27; E. Angelier et al. 1963: 464; M.-L. Angelier 1980: 13; E. Angelier et al. 1985: 30; Vinçon 1987: 240; Gerecke & Di Sabatino 1996: 313.
 New records. Gard: 0/2/0, Le TrŁvezet RiviŁre between l’Esperou and Meyrueis, 44°06.497 N 3°29.049 E, alt. 1115 m a.s.l., 16 May 2005, leg. H. Smit; 3/2/0, l’HØrault 3 km upstream of Valleraugue, 44°05.190 N 3°36.475 E, alt. 405 m a.s.l., 15 May 2005, leg. H. Smit.
Distribution in France: Corsica, Gard, Gers, Puy-de-Dôme, PyrØnØes (PyrØnØes-Atlantiques, PyrØnØes-Orientales, Hautes-PyrØnØes, AriŁge), Tarn.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on pages 45-46, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Spectral Variability of a Sample of Extreme Variability Quasars and Implications for the MgII Broad-line Region
Creators: name: Yang, Qian
name: Shen, Yue
name: Chen, Yu-Ching
name: Liu, Xin
name: Annis, James
name: Avila, Santiago
name: Bertin, Emmanuel
name: Brooks, David
name: Buckley-Geer, Elizabeth
name: Rosell, Aurelio Carnero
name: Kind, Matias Carrasco
name: Carretero, Jorge
name: da Costa, Luiz
name: Desai, Shantanu
name: Diehl, H. Thomas
name: Doel, Peter
name: Frieman, Josh
name: Garcia-Bellido, Juan
name: Gaztanaga, Enrique
name: Gerdes, David
name: Gruen, Daniel
name: Gruendl, Robert
name: Gschwend, Julia
name: Gutierrez, Gaston
name: Hollowood, Devon L.
name: Honscheid, Klaus
name: Hoyle, Ben
name: James, David
name: Krause, Elisabeth
name: Kuehn, Kyler
name: Lidman, Christopher
name: Lima, Marcos
name: Maia, Marcio
name: Marshall, Jennifer
name: Martini, Paul
name: Menanteau, Felipe
name: Miquel, Ramon
name: Malagon, Andres Plazas
name: Sanchez, Eusebio
name: Scarpine, Vic
name: Schindler, Rafe
name: Schubnell, Michael
name: Serrano, Santiago
name: Sevilla, Ignacio
name: Smith, Mathew
name: Soares-Santos, Marcelle
name: Sobreira, Flavia
name: Suchyta, Eric
name: Swanson, Molly
name: Tarle, Gregory
name: Vikram, Vinu
name: Walker, Alistair
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present new Gemini/GMOS optical spectroscopy of 16 extreme variability quasars (EVQs) that dimmed by more than 1.5 mag in the $g$ band between the Sloan Digital Sky Survey (SDSS) and the Dark Energy Survey (DES) epochs (separated by a few years in the quasar rest frame). The quasar sample covers a redshift range of $0.5 < z < 2.1$. Nearly half of these EVQs brightened significantly (by more than 0.5 mag in the $g$ band) in a few years after reaching their previous faintest state, and some EVQs showed rapid (non-blazar) variations of greater than 1-2 mag on timescales of only months. Leveraging on the large dynamic range in continuum variability between the earlier SDSS and the new GMOS spectra, we explore the associated variations in the broad Mg II,$\lambda2798$ line, whose variability properties have not been well studied before. The broad Mg II flux varies in the same direction as the continuum flux, albeit with a smaller amplitude, which indicates at least some portion of Mg II is reverberating to continuum changes. However, the width (FWHM) of Mg II does not vary accordingly as continuum changes for most objects in the sample, in contrast to the case of the broad Balmer lines. Using the width of broad Mg II to estimate the black hole mass therefore introduces a luminosity-dependent bias.
description: Submitted to MNRAS
Time-series Spectroscopy of Pulsating sdB Stars II: Velocity Analysis of PG1605+072
Creators: name: O'Toole, S. J.
name: Bedding, T. R.
name: Kjeldsen, H.
name: Dall, T. H.
name: Stello, D.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the analysis of time-resolved spectroscopy of the pulsating sdB star PG1605+072. From our main observing run of 16 nights we have detected velocity variations at 5 frequencies that correspond to those found in photometry. Based on these data, there appears to be change in amplitude of the dominant modes over about a year. However, when we include extra observations to improve the frequency resolution, we find that some of the frequencies are split into two or three. Simulations suggest that the apparent amplitude variation can be at least partially explained by a series of very closely spaced frequencies around the two strongest modes. By combining observations taken over ~300 days we conclude that some of the closely spaced modes are caused by one mode whose amplitude is varying, however this frequency is still within ~1 microHz of an apparently stable frequency. Because of this kind of complexity and uncertainty we advise caution when trying to identify oscillation modes in this star.
description: 12 pages, 13 figures, bibliography style file, accepted to MNRAS. Hi-resolution versions of figures 3 and 11 can be found at http://www.physics.usyd.edu.au/~otoole/papers/
Determination of reference intervals for nonesterified fatty acids in the blood serum of healthy dogs
Creators: name: Doll, Sophie-Charlotte K.
name: Haimerl, Peggy
name: Bartel, Alexander
name: Arlt, Sebastian Patrick
Publisher: name: Freie Universität Berlin
Year: 2022
Subjects: subject: Nonesterified fatty acids
subject: concentration
subject: blood serum
subject: 600 Technik, Medizin, angewandte Wissenschaften::630 Landwirtschaft::630 Landwirtschaft und verwandte Bereiche

description: Background Nonesterified fatty acids (NEFAs) are an important energy substrate in mammals. Measurement of the NEFA concentration in blood serum is common practice and enables reliable detection of a negative energy balance in several species. This parameter can be used to detect subclinical metabolic diseases or to optimise feeding to prevent severe negative energy balance. Since no reference values for dogs have been published, the aim of this study was to establish such values. Methods Blood serum from 85 healthy dogs was examined with a multiparameter clinical chemistry analyser. Given that NEFA values are not usually normally distributed, reference intervals (RIs) were calculated nonparametrically using bootstrapping (5000 replicates) for the 90% confidence intervals. Results The examined cohort had a median age of 62.16 months (2–180 months) and a median weight of 19.2 kg (3.0–55.0 kg) and comprised 27 (31.8%) males and 58 (68.2%) females, with 32 (37.6%) neutered or spayed. The fasting time was 5.9 h (range 0–23 h). The tested confounders age, sex, neuter status, bodyweight and body condition score did not significantly affect the NEFA concentrations. Conclusions The NEFA RI for dogs in this study was 0.2–1.47 mmol/L. The results may be used to adjust food composition and amount in healthy dogs or to detect metabolic disorders. Further research on NEFA metabolism in dogs maintained in standardised conditions and in specific nutritional situations or with particular diseases is warranted.
Limnesia (Limnesia) acuminata Walter 1925
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Limnesiidae
Limnesia
Limnesia acuminata

description: Limnesia (Limnesia) acuminata Walter, 1925
 Limnesia acuminata Walter, 1925: Migot 1926b: 111; Mota¸s & ¸ Soarec 1939a: Appendix; Dô 1962: 67.
 New record. HØrault: 0/1/0, Pool in dry river bed, tributary of La BuŁges near source, 43°49.180 N 3°35.254 E, 23 July 2008, leg. H. Smit & P. Martin.
Distribution in France: HØrault, PyrØnØes (PyrØnØes-Orientales).
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 47, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Seladerma nobile Delucchi 1955
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Seladerma
Seladerma nobile

description: Seladerma nobile Delucchi (Pteromalidae)
 Seladerma nobile Delucchi, 1955a: 47, 51. Holotype m, Germany (NMW [examined]).
 Material. HOLOTYPE m (cr, head, right antenna, left protarsus partly lacking, body glued with original micro-pin to card rectangle, left ¯agellum beyond ®fth segment glued beside rest of body) labelled`aberrans Frst [Novitzky’s handwriting]; TYPE [red]; SELADERMA nobile n. V. Delucchi det.’. One slide (sc) labelled`84; SELADERMA [black underlined] typus nobile [red underlined] antenna m; L. nobilis [sic] n. sp. antenna DIS [pasted over by former label]’ with right antenna of holotype.
 PARATYPES, NMW: 1 m (cr), 3 mm (mp, two pins) from the FoÈrster collection are considered as part of the type series. One slide (sc) labelled`82; SELADERMA [black underlined] nobile [red underlined] antenna m; 14 [circled] nobilis [sic] DIS [pasted over by former label]’ with right antenna (1955a: 50, ®gure 57) and one slide (sc) labelled`83; SELADERMA [black underlined] Typus nobile [red underlined] ala m; L. nobilis [sic] (Seladerma) [almost illegible] 14 [circled] DIS ala [pasted over by former label]’ with right fore wing (1955a: 50, ®gures 58, 59) of a further paratype female.
 Remarks. Delucchi described the female and stated`Type deÂposeÂ au MuseÂum d’Histoire Naturelle de Vienne...(speÂcimens coll. FoÈrster).’ but did not specify the number of specimens he had. The holotype clearly is a remounted specimen from the FoÈrster collection. The label`Typus’ on one of the above slides of a paratype is misleading in that it refers to the holotype which does not lack any wing. These slide-mounted parts which do not correspond to any of the paratypes seen and most probably stem from a single specimen are considered as part of the type series on the basis of the ®gures in the original publication.
 Examination of the relevant type series and a further 18 females and one male from Northern Europe (BMNH, VD) con®rmed the apparent synonymy of nobile with Seladerma laetum Walker as suggested by Graham (1969: 205).
 Status. Junior synonym of Seladerma laetum Walker syn. n.
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 103, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Additional file 14: of Genes, pathways and transcription factors involved in seedling stage chilling stress tolerance in indica rice through RNA-Seq analysis
Creators: name: Sharat Pradhan
name: Elssa Pandit
name: Nayak, Deepak
name: Lambodar Behera
name: Trilochan Mohapatra
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Table S8. Significant GO terms of early response phase (S1) of CSV genotype. (DOCX 17 kb)
Commensurability of graph products
Creators: name: Januszkiewicz, Tadeusz
name: Swiatkowski, Jacek
Publisher: name: arXiv
Year: 2001
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 20F65, 57M07

description: We define graph products of families of pairs of groups and study the question when two such graph products are commensurable. As an application we prove linearity of certain graph products.
description: Published by Algebraic and Geometric Topology at http://www.maths.warwick.ac.uk/agt/AGTVol1/agt-1-30.abs.html
Generalized Median Graph via Iterative Alternate Minimizations
Creators: name: Boria, Nicolas
name: Bougleux, S'ebastien
name: Gaüzère, Benoit
name: Brun, Luc
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: Computing a graph prototype may constitute a core element for clustering or classification tasks. However, its computation is an NP-Hard problem, even for simple classes of graphs. In this paper, we propose an efficient approach based on block coordinate descent to compute a generalized median graph from a set of graphs. This approach relies on a clear definition of the optimization process and handles labeling on both edges and nodes. This iterative process optimizes the edit operations to perform on a graph alternatively on nodes and edges. Several experiments on different datasets show the efficiency of our approach.
Limnesia (Limnesia) curvipalpis Tuzovskij 1997
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Limnesiidae
Limnesia
Limnesia curvipalpis

description: Limnesia (Limnesia) curvipalpis Tuzovskij, 1997
 New record. Pas-de-Calais: 0/2/0, pond, Les Landes de Blendecques, 50°42’1.46" N 2°14’10.91" E, 19 April 1996, leg. H. Smit & H. van der Hammen.
Distribution in France: Pas-de-Calais. New for the fauna of France.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 47, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
The compact central source in the RX J0852-4622 supernova remnant
Creators: name: Pavlov, G. G.
name: Sanwal, D.
name: Kiziltan, B.
name: Garmire, G. P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The central region of the recently discovered supernova remnant RX J0852.0-4622 was observed with the ACIS detector aboard the Chandra X-ray Observatory. We found only one relatively bright source, about 4' north of the SNR center, with a flux of $\sim 2\times 10^{-12}$ erg s$^{-1}$ cm$^{-2}$ in the 0.5--10 keV band. The position of this point-like source, CXOU J085201.4-461753, rules out its association with the two bright stars in the field, HD 76060 and Wray 16-30. Observations of the field with the CTIO 0.9-m telescope show a star ($R\approx 17$, $B\approx 19$) at about 2\farcs4 from the nominal X-ray position. We consider association of this star with the X-ray source unlikely and estimate a limiting magnitude of the optical counterpart as $B \ge 22.5$ and $R \ge 21.0$. Based on the X-ray-to-optical flux ratio, we argue that the X-ray source is likely the compact remnant of the supernova explosion that created the RX J0852.0-4622 SNR. The observed X-ray spectrum of the source is softer than spectra of magnetospheric radiation of rotation-powered pulsars, but it is harder than spectra of cooling neutron stars emitting thermal radiation from the entire surface, similar to the central compact source of the Cas A SNR. We suggest that CXOU J085201.4-461753 belongs to the growing family of radio-quiet compact central sources, presumably neutron stars, recently discovered in a number of SNRs.
description: 4 pages (incl. 2 embedded PS figures), AASTEX, uses emulateapj5.sty. Submitted to ApJ Letters
MOESM4 of Genotyping by low-coverage whole-genome sequencing in intercross pedigrees from outbred founders: a cost-efficient approach
Creators: name: Yanjun Zan
name: Payen, Thibaut
name: Lillie, Mette
name: Honaker, Christa
name: Siegel, Paul
name: ĂRjan Carlborg
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Additional file 4: Figure S4. Illustration of relationship between sequencing coverage, SNP density and imputation accuracy. (a/b) Histograms of the sequencing coverage/SNP densities for the 803 genotyped F2 individuals; (c/d) Scatter plots of individual coverage/SNP density vs imputation accuracy measured as proportion of sites that has same genotype with the averaged genotype probabilities estimated by Wahlberg et al. [21] using genotypes of 434 SNPs and microsatellite markers with the Haley and Knott algorithm [32].
What Kinds of Dogs Are Used in Clinical and Experimental Research?
Creators: name: Schulte, Evelyn
name: Arlt, Sebastian Patrick
Publisher: name: Freie Universität Berlin
Year: 2022
Subjects: subject: research dogs
subject: Beagles
subject: breed
subject: evidence-based medicine
subject: literature quality
subject: trial dogs
subject: 600 Technik, Medizin, angewandte Wissenschaften::630 Landwirtschaft::630 Landwirtschaft und verwandte Bereiche

description: Background: Dogs are widely used in research to answer questions about canine or human conditions. For the latter, research dogs are often used as models, since they are physiologically more similar to humans than other species used in research and they share similar environmental conditions. From a veterinary perspective, research findings are widely based on academic research, and thus are generated under experimental conditions. In that regard, the question arises: do the dogs used for research adequately represent the dog population seen in veterinary practice? It may, for example, be assumed that Beagle dogs are often used as experimental animals. The objective of this study was to evaluate the signalment of dogs used in veterinary research. Furthermore, we aimed to assess other relevant criteria regarding the validity of clinical trials in the context of six different veterinary medicine specialties: cardiology, internal medicine, neurology, orthopaedics, reproduction, and surgery. Methods: A literature search was conducted and 25 studies per specialty were randomly selected. The breed, sex, neuter status, median age, and median weight of the dogs used for clinical studies (n = 150) published between 2007 and 2019 were evaluated. Results: In total, 596,542 dogs were used in the 150 trials. Breed information was given for 33,835 of these dogs (5.7%). Of the latter, 1.9% were Beagles. Nine clinical trials exclusively used Beagles. The most frequently used breeds were German Shepherds (7.3%), Labrador Retrievers (6.7%), and Golden Retrievers (4.7%). The major reporting deficits found were missing breed specification in 25.3% of the articles; missing information about the sex of the dogs in 16.2%; missing age and weight information in 22.7 and 32.7%, respectively; and missing neuter status in 38.7% of the clinical studies. The median sample size was 56 (Q1:29; Q3:365) dogs. Conclusions: The presented project revealed that Beagle dogs represent only a small proportion of dogs in veterinary research. Based on the evaluated publications, it seems that some relevant dog attributes differ between the specialties. The results, however, show deficits in the reporting of demographic data for the dogs. The need for an improvement in the documentation and/or reporting of animal signalment is obvious and should be addressed by authors, reviewers, and journal editors in the future.
Seladerma violaceum Delucchi 1955
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Seladerma
Seladerma violaceum

description: Seladerma violaceum Delucchi (Pteromalidae)
 Seladerma violaceum Delucchi, 1955a: 47, 49. Holotype m, Germany (NMW [examined]).
 Material. HOLOTYPE m (mp, right ¯agellum, left hind wing, and right wings lacking, right hind leg and metasoma glued beside body on pith block) labelled`p. 439. 71. Or. Ex.. l; [empty label]; Collect. G. Mayr; Lamp. subviolaceus FoÈrster, Type; SELADERMA violaceum n. V. Delucchi det.; TYPE [red]’ (metanotum, propodeum, and metasoma illustrated, 1955a: 48, ®gure 56).
 Remarks. Delucchi described the female and stated`Type deÂposeÂ au MuseÂum d’Histoire Naturelle de Vienne’ but did not specify the number of specimens he had. The holotype is a specimen from the FoÈrster collection. Delucchi’s ®gure (see above) shows the gaster evenly symmetric whereas it is actually quite strongly shrivelled and deformed. According to Delucchi (pers. comm.) the outer form of a specimen has always been mirrored and made even, hence there is little doubt that the ®gure originates from the holotype.
 The holotype is a slightly aberrant specimen of Seladerma laetum Walker.
 Status. Junior synonym of Seladerma laetum Walker syn. n.
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 104, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Rigged configurations and the Bethe Ansatz
Creators: name: Schilling, Anne
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 82B23; 05A19; 05E10; 17B37

description: These notes arose from three lectures presented at the Summer School on Theoretical Physics "Symmetry and Structural Properties of Condensed Matter" held in Myczkowce, Poland, on September 11-18, 2002. We review rigged configurations and the Bethe Ansatz. In the first part, we focus on the algebraic Bethe Ansatz for the spin 1/2 XXX model and explain how rigged configurations label the solutions of the Bethe equations. This yields the bijection between rigged configurations and crystal paths/Young tableaux of Kerov, Kirillov and Reshetikhin. In the second part, we discuss a generalization of this bijection for the symmetry algebra $D_n^{(1)}$, based on work in collaboration with Okado and Shimozono.
description: 24 pages; lecture notes; axodraw style file required
Experimental Constraints on the Axion Dark Matter Halo Density
Creators: name: Asztalos, Stephen J.
name: Daw, E.
name: Peng, H.
name: Rosenberg, L. J
name: Hagmann, C.
name: Kinion, D.
name: Stoeffl, W.
name: van Bibber, K.
name: LaVeigne, J.
name: Sikivie, P.
name: Sullivan, N. S.
name: Tanner, D. B.
name: Nezrick, F.
name: Turner, Michael S.
name: Moltz, D. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Most of the mass of the Milky Way galaxy is contributed by its halo, presumably in the form of non-interacting cold dark matter. The axion is a compelling cold dark matter candidate. We report results from a search which probes the local galactic halo axion density using the Sikivie RF cavity technique. Candidates over the frequency range 550$$ $\le$ f $\le$$$ 810 MHz (2.3$$ $μ$eV $\le$$$ m$_{a}$ $\le$ 3.4 $μ$eV) were investigated. The absence of a signal suggests that KSVZ axions contribute no more than 0.45 GeV/cm$^3$ of mass density to the local dark matter halo over this mass range.
description: 10 pages (includes 3 figures)
Distribution of active forces in the cell cortex
Creators: name: Bohec, P.
name: Tailleur, J.
name: van Wijland, F.
name: Richert, A.
name: Gallet, F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: In this work, we study in detail the distribution of stochastic forces generated by the molecular motors activity, in the actin cortex of pre-muscular cells. By combining active and passive rheology experiments, performed on the same micro-bead bound to the actin network through membrane adhesive receptors, we measure the auto-correlation function Cff(t) of the average force pulling on the bead. Like for any out-of-equilibrium system, the force distribution differs from the thermodynamical equilibrium one, especially at long time scale t>1sec where the bead motion becomes partially directed. Thus the fluctuation-dissipation theorem does not apply and one can measure the distance from equilibrium through its violation. This work focuses on the influence of various parameters (ligand density, temperature, ATP depletion, molecular motors activity) on the force distribution. In particular, it is shown that the amplitude of active forces increases when the bead is more tighly attached to the cortex: this is interpreted through a model which takes into account the number of bonds between the bead and the cytoskeleton and the viscoelastic properties of the medium. It also increases with temperature, consistently with a description of the cell metabolism in terms of thermally activated reactions. Last, but not least, ATP depletion in the cell, or partial inhibitition of the actomyosin activity, leads to a decrease of the amplitude of the force distribution. Altogether, we propose a consistent and quantitative description for the motion of a micrometric probe interacting with the actin network, and for the amplitude of the stochastic forces generated by molecular motors in the cortex surrounding this probe.
Greenland Ice Sheet Surfaces Colonized by Microbial Communities Emit Volatile Organic Compounds
Creators: name: Doting, Eva L.
name: Davie-Martin, Cleo L.
name: Johansen, Anders
name: Benning, Liane G.
name: Tranter, Martyn
name: Rinnan, Riikka
name: Anesio, Alexandre Magno
Publisher: name: Freie Universität Berlin
Year: 2022
Subjects: subject: VOC
subject: glacier ice algae
subject: ice melt
subject: algal bloom
subject: cryoconite holes
subject: fungi
subject: biogenic volatiles
subject: red snow
subject: 500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::550 Geowissenschaften

description: Volatile organic compounds (VOCs) are emitted by organisms for a range of physiological and ecological reasons. They play an important role in biosphere–atmosphere interactions and contribute to the formation of atmospheric secondary aerosols. The Greenland ice sheet is home to a variety of microbial communities, including highly abundant glacier ice algae, yet nothing is known about the VOCs emitted by glacial communities. For the first time, we present VOC emissions from supraglacial habitats colonized by active microbial communities on the southern Greenland ice sheet during July 2020. Emissions of C5–C30 compounds from bare ice, cryoconite holes, and red snow were collected using a push–pull chamber active sampling system. A total of 92 compounds were detected, yielding mean total VOC emission rates of 3.97 ± 0.70 μg m–2 h–1 from bare ice surfaces (n = 31), 1.63 ± 0.13 μg m–2 h–1 from cryoconite holes (n = 4), and 0.92 ± 0.08 μg m–2 h–1 from red snow (n = 2). No correlations were found between VOC emissions and ice surface algal counts, but a weak positive correlation (r = 0.43, p = 0.015, n = 31) between VOC emission rates from bare ice surfaces and incoming shortwave radiation was found. We propose that this may be due to the stress that high solar irradiance causes in bare ice microbial communities. Acetophenone, benzaldehyde, and phenylmaleic anhydride, all of which have reported antifungal activity, accounted for 51.1 ± 11.7% of emissions from bare ice surfaces, indicating a potential defense strategy against fungal infections. Greenland ice sheet microbial habitats are, hence, potential sources of VOCs that may play a role in supraglacial microbial interactions, as well as local atmospheric chemistry, and merit future research efforts.
Polarisation of the Broad H alpha Wing in Symbiotic Stars
Creators: name: Yoo, Jerry Jaiyul
name: Bak, Jih-Yong
name: Lee, Hee-Won
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In many symbiotic stars there appear broad wings around H alpha, of which the formation mechanism proposed thus far includes a fast outflow, the inner accretion disc motion, electron scattering and Raman scattering of Ly beta. We adopt a Monte Carlo technique to simulate the Raman scattering of UV photons that are converted into optical photons around H alpha forming broad wings, and compute its polarisation. Noting that many symbiotic stars exhibit a bipolar nebular morphology and polarisation flip in the red wing part of the Raman scattered O {\tiny{VI}} features, we assume that the neutral scattering region is composed of the two components. The first component is a static cylindrical shell with finite thickness and the other component is a finite slab that is moving away with velocity v_p = 100 km s^{-1} along the symmetry axis of the first component. The cylindrical shell component yields polarisation in the direction parallel to the cylinder axis. The polarisation near the line-centre is weaker than in the far wing regions because of the large Rayleigh scattering numbers due to the large scattering cross sections near the line centre. The receding polar scattering component produces strong polarisation in the direction perpendicular to the cylinder axis. When the both scattering components coexist, the polarisation is characterised by weak parallel polarisation near the line-centre and strong perpendicular polarisation in the red part. We discuss the observational implications of our computation.
description: 14 pages, 8 figures. accepted for publication in MNRAS
Limnesia (Limnesia) undulatoides Davids 1997
Creators: name: Smit, H.
name: Gerecke, R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Limnesiidae
Limnesia
Limnesia undulatoides

description: Limnesia (Limnesia) undulatoides Davids, 1997
 New record: Pas-de-Calais: 1/2/0, pond dunes near Berck, 30 March 1990, leg. H. Smit.
Distribution in France: Pas-de-Calais. New for the fauna of France.
description: Published as part of Smit, H. & Gerecke, R., 2010, A CHECKLIST OF THE WATER MITES OF FRANCE (ACARI: HYDRACHNIDIA) Harry S and Reinhard G, pp. 21-91 in Acarologia 50 (1) on page 49, DOI: 10.1051/acarologia/20101952, http://zenodo.org/record/5392293
Cryptocurrency Smart Contracts for Distributed Consensus of Public Randomness
Creators: name: Mell, Peter
name: Kelsey, John
name: Shook, James
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Most modern electronic devices can produce a random number. However, it is difficult to see how a group of mutually distrusting entities can have confidence in any such hardware-produced stream of random numbers, since the producer could control the output to their gain. In this work, we use public and immutable cryptocurrency smart contracts, along with a set of potentially malicious randomness providers, to produce a trustworthy stream of timestamped public random numbers. Our contract eliminates the ability of a producer to predict or control the generated random numbers, including the stored history of random numbers. We consider and mitigate the threat of collusion between the randomness providers and miners in a second, more complex contract.
description: 16 pages, International Symposium on Stabilization, Safety, and Security of Distributed Systems
MOESM3 of Genotyping by low-coverage whole-genome sequencing in intercross pedigrees from outbred founders: a cost-efficient approach
Creators: name: Yanjun Zan
name: Payen, Thibaut
name: Lillie, Mette
name: Honaker, Christa
name: Siegel, Paul
name: ĂRjan Carlborg
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 3: Figure S3. Comparison of the founder mosaic in one F2 offspring obtained by using individual SNP-genotypes (a), to that obtained from our method (b) and STITCH (c) using the same low-coverage sequence data.
Concentrations of Dark Halos from their Assembly Histories
Creators: name: Wechsler, Risa H.
name: Bullock, James S.
name: Primack, Joel R.
name: Kravtsov, Andrey V.
name: Dekel, Avishai
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abridged) We study the relation between the density profiles of dark matter halos and their mass assembly histories, using a statistical sample of halos in a high-resolution N-body simulation of the LCDM cosmology. For each halo at z=0, we identify its merger-history tree, and determine concentration parameters c_vir for all progenitors, thus providing a structural merger tree for each halo. We fit the mass accretion histories by a universal function with one parameter, the formation epoch a_c, defined when the log mass accretion rate dlogM/dloga falls below a critical value S. We find that late forming galaxies tend to be less concentrated, such that c_vir ``observed'' at any epoch a_o is strongly correlated with a_c via c_vir=c_1*a_o/a_c. Scatter about this relation is mostly due to measurement errors in c_v and a_c, implying that the actual spread in c_vir for halos of a given mass can be mostly attributed to scatter in a_c. We demonstrate that this relation can also be used to predict the mass and redshift dependence of c_v, and the scatter about the median c_vir(M,z), using accretion histories derived from the Extended Press-Schechter (EPS) formalism, after adjusting for a constant offset between the formation times as predicted by EPS and as measured in the simulations;this new ingredient can thus be easily incorporated into semi-analytic models of galaxy formation. The correlation found between halo concentration and mass accretion rate suggests a physical interpretation: for high mass infall rates the central density is related to the background density; when the mass infall rate slows, the central density stays approximately constant and the halo concentration just grows as R_vir. The tight correlation demonstrated here provides an essential new ingredient for galaxy formation modeling.
description: 19 pages, 18 figures, uses emulateapj5.tex. ApJ, in press; revised to match accepted version
Moonraker: Enceladus Multiple Flyby Mission
Creators: name: Mousis, O.
name: Bouquet, A.
name: Langevin, Y.
name: André, Nicolas
name: Boithias, H.
name: Durry, G.
name: Faye, F.
name: Hartogh, P.
name: Helbert, J.
name: Iess, L.
name: Kempf, S.
name: Masters, A.
name: Postberg, Frank
name: Renard, J.-B.
name: Vernazza, P.
name: Vorburger, A.
name: Wurz, P.
name: Atkinson, D. H.
name: Barabash, S.
name: Berthomier, M.
name: Brucato, J.
name: Cable, M.
name: Carter, J.
name: Cazaux, S.
name: Coustenis, A.
name: Danger, G.
name: Dehant, V.
name: Fornaro, T.
name: Garnier, P.
name: Gautier, T.
name: Groussin, O.
name: Hadid, L. Z.
name: Ize, J.-C.
name: Kolmasova, I.
name: Lebreton, J.-P.
name: Maistre, S. Le
name: Lellouch, E.
name: Lunine, J. I.
name: Mandt, K. E.
name: Martins, Z.
name: Mimoun, D.
name: Nenon, Q.
name: Caro, G. M. Muñoz
name: Rannou, P.
name: Rauer, H.
name: Schmitt-Kopplin, P.
name: Schneeberger, A.
name: Simons, M.
name: Stephan, K.
name: Hoolst, T. Van
name: Vaverka, J.
name: Wieser, M.
name: Wörner, L.
Publisher: name: Freie Universität Berlin
Year: 2022
Subjects: subject: Enceladus
subject: moon
subject: Saturn
subject: 500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften

description: Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky core. Further investigation of the composition of the plume formed by the jets is necessary to fully understand the ocean, its potential habitability, and what it tells us about Enceladus’s origin. Moonraker has been proposed as an ESA M-class mission designed to orbit Saturn and perform multiple flybys of Enceladus, focusing on traversals of the plume. The proposed Moonraker mission consists of an ESA-provided platform with strong heritage from JUICE and Mars Sample Return and carrying a suite of instruments dedicated to plume and surface analysis. The nominal Moonraker mission has a duration of ∼13.5 yr. It includes a 23-flyby segment with 189 days allocated for the science phase and can be expanded with additional segments if resources allow. The mission concept consists of investigating (i) the habitability conditions of present-day Enceladus and its internal ocean, (ii) the mechanisms at play for the communication between the internal ocean and the surface of the South Polar Terrain, and (iii) the formation conditions of the moon. Moonraker, thanks to state-of-the-art instruments representing a significant improvement over Cassini's payload, would quantify the abundance of key species in the plume, isotopic ratios, and the physical parameters of the plume and the surface. Such a mission would pave the way for a possible future landed mission.
Skeloceras cerebrosum Delucchi 1955
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Pteromalidae
Skeloceras
Skeloceras cerebrosum

description: Skeloceras cerebrosum Delucchi (Pteromalidae)
 Skeloceras cerebrosum Delucchi, 1955a: 21, 24. Holotype m, Germany (NMW [examined]).
 Material. HOLOTYPE m (cr, left pedicel with ¯agellum, right ¯agellum beyond ®rst segment, and left fore leg beyond trochanter lacking, body glued with original micro-pin to card rectangle) labelled`p. 232. o. Or. Ex. m.; [empty label]; Collect. G. Mayr; Lamp. sulcatulus FoÈrster, Type; [cp, yellow]; SKELOCERAS cerebrosum n. V. Delucchi det.; TYPE [red]’.
 Remarks. Delucchi described the female and stated`Type deÂposeÂ au MuseÂum d’Histoire Naturelle de Vienne.’ but did not specify the number of specimens he had. Holotype subsequently remounted from micro-pin by me. It is a specimen from the FoÈrster collection. One male (dp) in the NMW provided only with Delucchi’s identi®cation label is not considered as part of the type series, since the male was not described.
 Delucchi (1955a: 21) separated cerebrosum from Lamprotatus truncatus (Fonscolombe) [sub Skeloceras mirabile Delucchi] by diOEerences in the sculpture of the propodeum. Examination of 25 females and 16 males from Northern and Central Europe, Croatia, France, and Italy (BMNH, MG, MHNG, MZL, NMBE, NMW, VD, ZB) showed that this character is quite variable. The sculpture consists of some oblique striae which sometimes may indicate an irregular median carina or a costula, though the latter is never as distinct as e.g. in L. novickyi (Delucchi). With regard to this variation cerebrosum certainly lies within the range of variation of truncatus.
 Status. Junior synonym of Lamprotatus (Skeloceras) truncatus (Fonscolombe) syn. n.
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 104, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
No evidence for intermediate-mass black holes in the globular clusters $ω$ Cen and NGC 6624
Creators: name: Baumgardt, Holger
name: He, Chenyu
name: Sweet, Sarah M.
name: Drinkwater, Michael
name: Sollima, Antonio
name: Hurley, Jarrod
name: Usher, Christopher
name: Kamann, Sebastian
name: Dalgleish, Hannah S.
name: Dreizler, Stefan
name: Husser, Tim-Oliver
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We compare the results of a large grid of N-body simulations with the surface brightness and velocity dispersion profiles of the globular clusters $ω$ Cen and NGC 6624. Our models include clusters with varying stellar-mass black hole retention fractions and varying masses of a central intermediate-mass black hole (IMBH). We find that an $\sim 45,000$ M$_\odot$ IMBH, whose presence has been suggested based on the measured velocity dispersion profile of $ω$ Cen, predicts the existence of about 20 fast-moving, $m>0.5$ M$_\odot$ main-sequence stars with a (1D) velocity $v>60$ km/sec in the central 20 arcsec of $ω$ Cen. However no such star is present in the HST/ACS proper motion catalogue of Bellini et al. (2017), strongly ruling out the presence of a massive IMBH in the core of $ω$ Cen. Instead, we find that all available data can be fitted by a model that contains 4.6% of the mass of $ω$ Cen in a centrally concentrated cluster of stellar-mass black holes. We show that this mass fraction in stellar-mass BHs is compatible with the predictions of stellar evolution models of massive stars. We also compare our grid of $N$-body simulations with NGC 6624, a cluster recently claimed to harbor a 20,000 M$_\odot$ black hole based on timing observations of millisecond pulsars. However, we find that models with $M_{IMBH}>1,000$ M$_\odot$ IMBHs are incompatible with the observed velocity dispersion and surface brightness profile of NGC 6624,ruling out the presence of a massive IMBH in this cluster. Models without an IMBH provide again an excellent fit to NGC 6624.
description: 14 pages, 6 figures, accepted for publication in MNRAS