cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of Rate of individuals with clearly increased radiosensitivity rise with age both in healthy individuals and in cancer patients
Creators: name: Schuster, Barbara
name: Ellmann, Anna
name: Mayo, Theresa
name: Auer, Judith
name: Haas, Matthias
name: Hecht, Markus
name: Fietkau, Rainer
name: Distel, Luitpold
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S1. Three color fluorescence in situ hybridization of three chromosomes to determine radiosensitivity. Chromosome # 1 (red, rhodamine), chromosome # 2 (green, FITC) and chromosome # 4 (yellow, rhodamine + FITC) were painted with chromosome specific probes. DNA was stained with DAPI (blue) (A-D). The first row shows an overlay of the color images. In the second row are black and white images of the red painted chromosomes, in the third row of the green painted chromosomes. The last row displays all chromosomes of the blue stain as black and white images. All aberrations are marked in each color image where they occur. A normal metaphase spread is shown in (A). Metaphase spread with two translocations of # 2 with a blue chromosome and # 4 with a blue chromosome and an insertion of # 1 into a blue chromosome. The three aberrations were scored as 7 breaks (B). Metaphase spread with a dicentric chromosome of # 1 and # 2, a translocation of # 1 and # 4 and an insertion of # 1, # 2 and # 4. The aberrations were scored as 5 breaks (C). Metaphase spread with complex chromosomal rearrangements (CCR). The aberrations were scored as 12 breaks. The breaks of the red chromosome are marked with an arrow, of the green chromosome with an arrowhead and of the yellow one with a concave arrowhead (D). Scale: 10Â Îźm. (PDF 947 kb)
Primordial non-Gaussianity with $μ$-type and $y$-type spectral distortions: exploiting Cosmic Microwave Background polarization and dealing with secondary sources
Creators: name: Ravenni, Andrea
name: Liguori, Michele
name: Bartolo, Nicola
name: Shiraishi, Maresuke
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Cross-correlations between Cosmic Microwave Background (CMB) temperature and $y$-spectral distortions anisotropies have been previously proposed as a way to measure the local bispectrum parameter $f_{\rm NL}^{\rm loc.}$ in a range of scales inaccessible to either CMB ($T$, $E$) bispectra or $T$-$μ$ correlations. This is useful e.g. to test scale dependence of primordial non-Gaussianity. Unfortunately, the primordial $y$-T signal is strongly contaminated by the late-time correlation between the Integrated Sachs Wolfe and Sunyaev-Zel'dovich (SZ) effects. Moreover, SZ itself generates a large noise contribution in the $y$-parameter map. We consider two original ways to address these issues. In order to remove the bias due to the SZ-CMB temperature coupling, while also adding new signal, we include in the analysis the cross-correlation between $y$-distortions and CMB {\em polarization}. In order to reduce the noise, we propose to clean the $y$-map by subtracting a SZ template, reconstructed via cross-correlation with external tracers (CMB and galaxy-lensing signals). We combine this SZ template subtraction with the previously adopted solution of directly masking detected clusters. Our final forecasts show that, using $y$-distortions, a PRISM-like survey can achieve $1σ(f_{\rm NL}^\text{loc.}) = 300$, while an ideal experiment will achieve $1σ(f_{\rm NL}^\text{loc.}) = 130$, with improvements of a factor $\sim 3$ from adding the $y$-$E$ signal, and a further $20-30 \%$ from template cleaning. These forecasts are much worse than current $f_{\rm NL}^\text{loc.}$ boundaries from {\em Planck}, but we stress again that they refer to completely different scales.
description: 24 pages, 5 figures
High order correlation functions for self interacting scalar field in de Sitter space
Creators: name: Bernardeau, Francis
name: Brunier, Tristan
name: Uzan, Jean-Philippe
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present the expressions of the three- and four-point correlation functions of a self interacting light scalar field in a de Sitter spacetime at tree order respectively for a cubic and a quartic potential. Exact expressions are derived and their limiting behaviour on super-horizon scales are presented. Their essential features are shown to be similar to those obtained in a classical approach.
description: 8 pages, 4 figures
Electrostatically tunable adhesion in a high speed sliding interface
Creators: name: Rajauria, Sukumar
name: Ruiz, Oscar
name: Canchi, Sripathi V.
name: Schreck, Erhard
name: Dai, Qing
Publisher: name: arXiv
Year: 2017
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Contact hysteresis between sliding interfaces is a widely observed phenomenon from macro- to nano- scale sliding interfaces. Most of such studies are done using an atomic force microscope (AFM) where the sliding speed is a few μm/s. Here, we present a unique study on stiction between the head-disk interface of commercially available hard disk drives, wherein vertical clearance between the head and the disk is of the same order as in various AFM based fundamental studies, but with a sliding speed that is nearly six orders of magnitude higher. We demonstrate that although the electrostatic force (DC or AC voltage) is an attractive force, the AC voltage induced out-of-plane oscillation of the head with respect to disk is able to suppress completely the contact hysteresis.
description: 5 pages, 4 figures
Generalized uncertainty principle and correction value to the black hole entropy
Creators: name: Hai-Xia, Zhao
name: Huai-Fan, Li
name: Shuang-Qi, Hu
name: Ren, Zhao
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Recently, there has been much attention devoted to resolving the quantum corrections to the Bekenstein-Hawking entropy of the black hole. In particular, many researchers have expressed a vested interest in the coefficient of the logarithmic term of the black hole entropy correction term. In this paper, we calculate the correction value of the black hole entropy by utilizing the generalized uncertainty principle and obtain the correction term caused by the generalized uncertainty principle. Because in our calculation we think that the Bekenstein-Hawking area theorem is still valid after considering the generalized uncertainty principle, we derive that the coefficient of the logarithmic term of the black hole entropy correction term is negative. This result is different from the known result at present. Our method is valid not only for single horizon spacetime but also for double horizons spacetime. In the whole process, the physics idea is clear and calculation is simple. It offers a new way for studying the condition that Bekenstein-Hawking area theorem is valid.
Limnomedusae Kramp 1938
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Limnomedusae

description: Order Limnomedusae Kramp, 1938  Limnomedusae Kramp, 1938: 107.
 Diagnosis. Hydrozoa with polyps solitary or primitively colonial; hydranths small to minute, morphologically simple, sessile, lacking hydrothecae; hypostome, mouth, and gastric cavity present or absent; tentacles and perisarcal sheath present or absent; asexual reproduction frequent, by frustules, or frustule-like buds, or cysts.
Gonophores fixed or free eumedusoids, or medusae. Medusae, when present, with hemispherical to discoidal umbrella; tentacles hollow, lacking basal bulbs; marginal sense organs, when present, comprising internal statocysts; gonads on radial canals or manubrium.
 Remarks. The history and phylogeny of Limnomedusae Kramp, 1938 has been reviewed by Daly et al. (2007) and Collins et al. (2008). Bouillon et al. (2006) included 21 genera in the family, many of them poorly known (Jankowski 2001) and over half (12) being monotypic.
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 72, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
title: 02_1117
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
An introduction to random matrix theory
Creators: name: Borot, Gaëtan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 15B52, 60B20, 62-07

description: These are lectures notes for a 4h30 mini-course held in Ulaanbaatar, National University of Mongolia, August 5-7th 2015, at the summer school "Stochastic Processes and Applications". It aims at presenting an introduction to basic results of random matrix theory and some of its motivations, targeted to a large panel of students coming from statistics, finance, etc. Only a small background in probability is required.
description: 55 pages, 10 figures
Craspedacusta Lankester 1880
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Limnomedusae
Olindiidae
Craspedacusta

description: Genus Craspedacusta Lankester, 1880
 Craspedacusta Lankester, 1880: 147.
 Type species. Craspedacusta sowerbii Lankester, 1880, by monotypy.
 Diagnosis. Olindiid polyps solitary or primitively colonial. Hydranths atentaculate, athecate, club-shaped to cylindrical; distal end a knob-shaped capitulum, bearing an apical mouth surrounded by nematocysts; hydranth base with attachment region surrounded by thin perisarc; asexual reproduction by frustulation, cyst formation, or fission.
Gonophores medusae, arising from gastric column of hydranth. Medusae hemispherical to dome-shaped, with marginal nematocyst ring; radial canals four; centripetal canals absent; manubrium quadrate, moderately short, gastric peduncle absent; tentacles evenly spaced, of one type, lacking adhesive disks; statocysts in vesicles on velum; gonads sac-shaped, on radial canals.
 Remarks. Bouillon et al. (2006) listed eight nominal species in Craspedacusta Lankester, 1880, but speculated that they might all be conspecific with C. sowerbii Lankester, 1880. Earlier, He et al. (2000) had recognized six species, while Dumont (1994) reported that four species were considered valid by most workers. Jankowski (2001) and Jankowski et al. (2008) believed there were as many as four species endemic to the Yangtze River Basin in China, the likely origin of the genus. Several species of the genus appear valid from molecular data (Collins et al. 2008; Zhang et al. 2009). The species taxonomy of this enigmatic fresh water genus remains unsettled.
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on pages 73-74, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Clues on galaxy and cluster formation from their scaling relations
Creators: name: Lanzoni, B.
name: Ciotti, L.
name: Cappi, A.
name: Tormen, G.
name: Zamorani, G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: By means of high-resolution N-body simulations in a LambdaCDM cosmology, we verify that scaling relations similar to those observed for nearby galaxy clusters are also defined by their dark matter hosts; the slopes, however, are not the same. We then show that the scaling relations of galaxy clusters can be explained as the result of the cosmological collapse of density fluctuations at the appropriate scales, plus a systematic trend of the M/L ratio with cluster mass. The empirical fact that the exponent of the Faber-Jackson relation of elliptical galaxies is significantly different (higher) than that of clusters, force us to conclude that the galaxy scaling laws might derive from the cosmological collapse of density fluctuations at the epoch when galactic scales became non-linear, plus modifications afterward due to early-time dissipative merging.
description: 2 pages, 1 fig., in press on the Proceedings of the ESO-USM-MPE Workshop "Multiwavelength mapping of galaxy formation and evolution", ESO Astrophysics Symposia, R. Bender and A. Renzini eds
Additional file 7: of Homoeolog expression bias in allopolyploid oleaginous marine diatom Fistulifera solaris
Creators: name: Nomaguchi, Tatsuhiro
name: Maeda, Yoshiaki
name: Yoshino, Tomoko
name: Asahi, Toru
name: Tirichine, Leila
name: Bowler, Chris
name: Tanaka, Tsuyoshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology

description: Figure S6. GO terms of consistently biased homoeologous genes. Figure shows the frequency of GO terms, annotated to the second depth, within the group of homoeologous genes which were consistently biased towards Fso_h or Fso_l (corresponding to the genes in the histogram of Fig.Â 3b). Orange and blue colors represent the direction of homoeolog expression bias of the group, Fso_h and Fso_l, respectively. Dots in the figure represent the log ratio of frequency of corresponding GO terms between Fso_h-biased group and Fso_l-biased group. (PDF 279 kb)
Absorption by cold Fermi atoms in a harmonic trap
Creators: name: Juzeliunas, Gediminas
name: Masalas, Marius
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the absorption spectrum for a strongly degenerate Fermi gas confined in a harmonic trap. The spectrum is calculated using both the exact summation and also the Thomas-Fermi (TF) approximation. In the latter case, relatively simple analytical expressions are obtained for the absorption lineshape at large number of trapped atoms. At zero temperature, the approximated lineshape is characterized by a $(1-z^2)^{5/2}$ dependence which agrees well with the exact numerical calculations. At non-zero temperature, the spectrum becomes broader, although remains non-Gaussian as long as the fermion gas is degenerate. The changes in the trap frequency for an electronically excited atom can introduce an additional line broadening.
description: 4 pages, 5 figures
Additional file 6: of Overexpression of the protein disulfide isomerase AtCYO1 in chloroplasts slows dark-induced senescence in Arabidopsis
Creators: name: Tominaga, Jun
name: Nakahara, Yasutoshi
name: Horikawa, Daisuke
name: Tanaka, Ayumi
name: Kondo, Maki
name: Kamei, Yasuhiro
name: Takami, Tsuneaki
name: Sakamoto, Wataru
name: Unno, Kazutoshi
name: Sakamoto, Atsushi
name: Shimada, Hiroshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Plant Biology

description: Figure S3. Ultrastructure of chloroplasts at 10 DDI. (PDF 3868Â kb)
Cooling timescale of dust tori in dying active galactic nuclei
Creators: name: Ichikawa, Kohei
name: Tazaki, Ryo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We estimate the dust torus cooling timescale once the active galactic nucleus (AGN) is quenched. In a clumpy torus system, once the incoming photons are suppressed, the cooling timescale of one clump from $T_{\rm dust}=1000$ K to several $10$ K is less than $10$ years, indicating that the dust torus cooling time is mainly governed by the light crossing time of the torus from the central engine. After considering the light crossing time of the torus, the AGN torus emission at $12~μ$m becomes over two orders of magnitude fainter within $100$ years after the quenching. We also propose that those "dying" AGN could be found using the AGN indicators with different physical scale $R$ such as $12~μ$m band luminosity tracing AGN torus ($R \sim 10$ pc) and the optical [OIII]$\lambda5007$ emission line narrow line regions ($R=10^{2-4}$ pc).
description: 8 pages, 4 figures, accepted for publication in ApJ
Brightest cluster galaxy formation in the cluster C0037-2522: flattening of the dark matter cusp
Creators: name: Nipoti, C.
name: Stiavelli, M.
name: Ciotti, L.
name: Treu, T.
name: Rosati, P.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The X-ray cluster C0337-2522 at redshift $z=0.59$ hosts in its core a group of five elliptical galaxies. Using N-body simulations we show that a multiple merging event among the five galaxies is expected to take place in the next few Gyrs, forming a central brightest cluster galaxy. We also find indications that dynamical friction heating associated with this event is likely to modify the central slope of the cluster dark matter density profile.
description: 2 pages, 1 fig., in press on the Proceedings of the ESO-USM-MPE Workshop "Multiwavelength mapping of galaxy formation and evolution", ESO Astrophysics Symposia, R. Bender and A. Renzini eds
title: Disproportionate Collapse Analysis of Cable-stayed Steel Roofs for Cable Loss
Creators: name: Gerasimidis, Simos
name: Baniotopoulos, C.
Publisher: name: University of Massachusetts Amherst
Year: 2011
Subjects: subject: cable-stayed structure
subject: robustness
subject: disproportionate collapse
subject: cable loss
subject: dynamic amplification factors
subject: load increase factors
subject: Civil and Environmental Engineering
subject: Engineering

description: Disproportionate collapse has been identified lately as a real cause of failure for structural engineering projects. Rare and unexpected, the phenomenon of disproportionate collapse usually results to many fatalities and thus, its analysis and mitigation is deemed necessary. This work describes the analysis of a cable-stayed steel roof under the scenario of a cable loss. The eventof a cable loss is assumed to be brittle, while relevant recent recommendations suggest the application of a scaled equivalent static force at the points of the anchorage of the cable but in the opposite direction of the original cable force. In this paper, three different conditions have been considered in order to study the effect of the cable loss into the overall structural responseof a typical cable-stayed roof; the level of the equivalent nodal load in the opposite direction of the original cable force varies. The steel structure of the roof, in its complexity, closer to responding as a cable-stayed bridge rather than a steel roof provides a useful template for conclusions; several topics regarding disproportionate collapse and cable losses are discussed.
Craspedacusta sowerbii Lankester 1880
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Limnomedusae
Olindiidae
Craspedacusta
Craspedacusta sowerbii

description: Craspedacusta sowerbii Lankester, 1880
Fig. 48
 Craspedacusta sowerbii Lankester, 1880: 148.
 Craspedacusta sowerbyi.— Edmondson, 1940: 314 [medusa only].— Matthews, 1963: 18, figs. 1, 2; 1966: 246, figs. 1–5.
 Type locality. UK: London, Regent’s Park, “…in the tank in the water-lily house…” (Lankester 1880: 147).
 Material examined. None.
 Description. As for diagnosis of genus.
 Remarks. Craspedacusta sowerbii Lankester, 1880 is a well-known freshwater species with a wide geographic range (Kramp 1961; Dumont 1994). Edmondson (1940) first reported the species from Hawaii, based on medusae found at Maliko Gulch, Maui. Both medusa and polyp stages were later reported from Honolulu in aquaria by Matthews (1963, 1966). No specimens of the hydroid were found in collections at the Bishop Museum, and it is not currently known to occur in limnic aquaria and culture systems at the Waikiki Aquarium (Gerald Crow & Kelley Lam, pers. comm., 30 July 2009).
 A review of the global distribution, dispersal, and feeding ecology of C. sowerbii and other freshwater medusae is given by Dumont (1994).
 Reported distribution. Hawaii. Maui: Maliko Gulch [medusa only] (Edmondson 1940).–Oahu: Honolulu, in aquaria (Matthews 1963, 1966).
 Worldwide. All continents except Antarctica, in shallow subtropical and temperate fresh waters (Kramp 1961; Dumont 1994; Jankowski 2001; Jankowski et al. 2008; Zhang et al. 2009).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 74, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
QUANTIFICATION OF RADIONUCLIDE LEVELS IN HORSE CHESTNUT SEEDS
Creators: name: Yokubova, Nilufar
Publisher: name: Zenodo
Year: 2024

description: Radionuclides are unstable forms of elements that emit radiation, and they are hazardous pollutants that can have a significant impact on the environment, the food chain, and human health. These substances persist in the environment for a long time, potentially causing soil, water, and air contamination, which poses risks to ecosystems and human populations. When present in soil and groundwater, radionuclides can be absorbed by plants, leading to potential radiation exposure for people who consume contaminated plant parts. Therefore, it is important to analyze the radionuclide content in the seeds of horse chestnuts grown in different regions.
title: Calendrier des ateliers du numérique du 1er semestre 2014
Creators: name: LabexMed
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017

description: Calendrier des ateliers du numérique du 1er semestre 2014
[O II] nebular emission from Mg II absorbers: Star formation associated with the absorbing gas
Creators: name: Joshi, Ravi
name: Srianand, Raghunathan
name: Petitjean, Patrick
name: Noterdaeme, Pasquier
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present nebular emission associated with 198 strong Mg II absorbers at 0.35 $\le z \le$ 1.1 in the fibre spectra of quasars from the Sloan Digital Sky Survey. Measured [O II] luminosities (L$_{[O II]}$) are typical of sub-L$^{\star}$ galaxies with derived star formation rate (uncorrected for fibre losses and dust reddening) in the range of 0.5-20 ${\rm M_\odot\ yr^{-1}}$. Typically less than $\sim$ 3% of the Mg II systems with rest equivalent width, $W_{2796}$ $\ge$ 2 Å, show L$_{[O II]} \ge 0.3$ L$^{\star}_{[O II]}$. The detection rate is found to increase with increasing $W_{2796}$ and $z$. No significant correlation is found between $W_{2796}$ and L$_{[O II]}$ even when we restrict the samples to narrow $z$-ranges. A strong correlation is seen between L$_{[O II]}$ and $z$. While this is expected from the luminosity evolution of galaxies, we show finite fibre size plays a very crucial role in this correlation. The measured nebular line ratios (like [O III]/[O II] and [O III]/H$β$) and their $z$ evolution are consistent with those of galaxies detected in deep surveys. Based on the median stacked spectra, we infer the average metallicity (log Z $\sim$8.3), ionization parameter (log $q$ $\sim$7.5) and stellar mass (log (M/M$_\odot$)$\sim$9.3). The Mg II systems with nebular emission typically have $W_{2796}$ $\ge 2$ Å, Mg II doublet ratio close to 1 and W(Fe II$λ$2600)/$W_{2796}$ $\sim 0.5$ as often seen in damped Ly$α$ and 21-cm absorbers at these redshifts. This is the biggest reported sample of [O II] emission from Mg II absorbers at low impact parameters ideally suited for probing various feedback processes at play in $z\le 1$ galaxies.
description: 18 Pages, 18 Figures, 4 Tables (Accepted for the Publication in MNRAS main-journal)
Additional file 6: of Homoeolog expression bias in allopolyploid oleaginous marine diatom Fistulifera solaris
Creators: name: Nomaguchi, Tatsuhiro
name: Maeda, Yoshiaki
name: Yoshino, Tomoko
name: Asahi, Toru
name: Tirichine, Leila
name: Bowler, Chris
name: Tanaka, Tsuyoshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Figure S5. Homoeolog expression bias in highly expressing genes. (A) Box plot showing RPKM values of homoeologous genes at each time point. The minimum value of outlier (represented as a circle in the figure) is approximately 50 at every time point. (B-D) Histograms show number of homoeologous genes expressing in a biased fashion towards a specific subgenome. Each figure includes the homoeologous genes expressing within a certain range of RPKM values; (B) RPKM >â 50, (C) >â 100 and (D) >â 500. N values in figure represent the number of genes expressing preferentially in subgenome A or B. S values in the figure indicate the number of genes counted as biased expression due to silencing of the other homoeologous pair (not included in histograms). (PDF 97 kb)
Additional file 2 of Targeting the inward rectifier potassium channel 5.1 in thyroid cancer: artificial intelligence-facilitated molecular docking for drug discovery
Creators: name: Yang, Xue
name: Wu, Yonglin
name: Xu, Shaojie
name: Li, Hanning
name: Peng, Chengcheng
name: Cui, Xiaoqing
name: Dhoomun, Deenraj Kush
name: Wang, Ge
name: Xu, Tao
name: Dong, Menglu
name: Li, Xingrui
name: Du, Yaying
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Supplementary Material 2
Phantom fields: bounce solutions in the early Universe and S-branes
Creators: name: Dzhunushaliev, Vladimir
name: Folomeev, Vladimir
name: Myrzakulov, Kairat
name: Myrzakulov, Ratbay
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The cosmological model with two phantom scalar fields with the special choice of field's potential is considered. The obtained regular solution describes a bounce with a subsequent transition to the de Sitter stage of the expansion of the Universe. This solution also could be interpreted as a S-brane solution.
description: one reference and new interpretation of the solution are added, and the title is changed
Primitive Equations with Linearly Growing Initial Data
Creators: name: Hussein, Amru
name: Saal, Martin
name: Sawada, Okihiro
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35Q35 (Primary), 76D03, 47D06, 35K65, 86A05 (Secondary)

description: The primitive equations in a 3D infinite layer domain are considered with linearly growing initial data in the horizontal direction, which illustrates the global atmospheric rotating or straining flows. On the boundaries, Dirichlet, Neumann or mixed boundary conditions are imposed. The Ornstein-Uhlenbeck type operator appears in the linear parts, so the semigroup theory is established by Trotter's arguments due to decomposition of infinitesimal generators. To obtain smoothing properties of the semigroup, derivatives of the associated kernel are calculated. For proving time-local existence and uniqueness of mild solutions, the adapted Fujita-Kato scheme is used in certain Sobolev spaces.
description: 16 pages
Curvaton Dynamics in Brane-worlds
Creators: name: Papantonopoulos, Eleftherios
name: Zamarias, Vassilios
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the curvaton dynamics in brane-world cosmologies. Assuming that the inflaton field survives without decay after the end of inflation, we apply the curvaton reheating mechanism to Randall-Sundrum and to its curvature corrections: Gauss-Bonnet, induced gravity and combined Gauss-Bonnet and induced gravity cosmological models. In the case of chaotic inflation and requiring suppression of possible short-wavelength generated gravitational waves, we constraint the parameters of a successful curvaton brane-world cosmological model. If density perturbations are also generated by the curvaton field then, the fundamental five-dimensional mass could be much lower than the Planck mass
description: 47 pages, 1 figure, references added, to be published in JCAP
Calpasoma Fuhrmann 1939
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Limnomedusae
Olindiidae
Calpasoma

description: Genus Calpasoma Fuhrmann, 1939
 Calpasoma Fuhrmann, 1939: 363.
 Type species. Calpasoma dactylopterum Fuhrmann, 1939, by monotypy.
 Diagnosis. Olindiid polyps solitary, although bipolar or tripolar forms sometimes present. Hydranths minute, athecate, sausage-shaped to cylindrical, with distal mouth but without prominent capitulum; tentacles usually present distally, appearing to arise in two close whorls or irregularly arranged, each tentacle a slender and filiform protrusion of an epithelial tentaculocyte; several nematocysts on distal end of each tentacle, scattered elsewhere; asexual reproduction by frustulation or budding.
Gonophores not known.
 Remarks. Calpasoma Fuhrmann, 1939 is a peculiar freshwater hydrozoan genus, sometimes believed to be merely a tentaculate form of Craspedacusta Lankester, 1880. Studies such as those of Matthews (1966), and Rahat & Campbell (1974), support recognition of the two as distinct, although Jankowski (2001) considered at least one form of Calpasoma to be congeneric with Craspedacusta. Astrohydra Hashimoto, 1981 appears similar, but the genus (and its type species, A. japonica Hashimoto, 1981) is not well-known.
 The generic name Calpasoma is neuter (ICZN Art. 30.1.2), and the specific name of its single contained species should be spelled dactylopterum, not dactyloptera as originally formed.
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on pages 74-75, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Hiding bits in Bell states
Creators: name: Terhal, Barbara M.
name: DiVincenzo, David P.
name: Leung, Debbie W.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a scheme for hiding bits in Bell states that is secure even when the sharers Alice and Bob are allowed to carry out local quantum operations and classical communication. We prove that the information that Alice and Bob can gain about a hidden bit is exponentially small in $n$, the number of qubits in each share, and can be made arbitrarily small for hiding multiple bits. We indicate an alternative efficient low-entanglement method for preparing the shared quantum states. We discuss how our scheme can be implemented using present-day quantum optics.
description: 4 pages RevTex, 1 figure, various small changes and additional paragraph on optics implementation
Bright X-ray flares from Sgr A*
Creators: name: Karssen, G. D.
name: Bursa, M.
name: Eckart, A.
name: Valencia-S., M.
name: Dovciak, M.
name: Karas, V.
name: Horak, J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We address a question whether the observed light curves of X-ray flares originating deep in galactic cores can give us independent constraints on the mass of the central supermassive black hole. To this end we study four brightest flares that have been recorded from Sagittarius A*. They all exhibit an asymmetric shape consistent with a combination of two intrinsically separate peaks that occur at a certain time-delay with respect to each other, and are characterized by their mutual flux ratio and the profile of raising/declining parts. Such asymmetric shapes arise naturally in the scenario of a temporary flash from a source orbiting near a super- massive black hole, at radius of only 10-20 gravitational radii. An interplay of relativistic effects is responsible for the modulation of the observed light curves: Doppler boosting, gravitational redshift, light focusing, and light-travel time delays. We find the flare properties to be in agreement with the simulations (our ray-tracing code sim5lib). The inferred mass for each of the flares comes out in agreement with previous estimates based on orbits of stars; the latter have been observed at radii and over time-scales two orders of magnitude larger than those typical for the X-ray flares, so the two methods are genuinely different. We test the reliability of the method by applying it to another object, namely, the Seyfert I galaxy RE J1034+396.
description: MNRAS in press; 12 pages; 9 figures; 3 tables Accepted 2017 September 4. Received 2017 September 4; in original form 2017 May 22; minor changes applied
X-ray and radio prompt emission from a hypernova SN 2002ap
Creators: name: Chandra, P.
name: Ray, A.
name: Sutaria, F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Here we report on combined X-ray and radio observations of SN 2002ap with XMM-Newton ToO observation and GMRT observations aided with VLA published results. In deriving the X-ray flux of SN 2002ap we account for the contribution of a nearby source, found to be present in the pre-SN explosion images obtained with Chandra observatory. We also derive upper limits on mass loss rate from X-ray and radio data. We suggest that the prompt X-ray emission is non-thermal in nature and its is due to the repeated compton boosting of optical photons. We also compare SN's early radiospheric properties with two other SNe at the same epoch.
description: 4 pages, 5 figures. Uses espcrc2.sty. To appear in proceedings of symposium on X-ray astronomy "The Restless High-Energy Universe", May 2003, Amsterdam, The Netherlands, eds. E.P.J. van den Heuvel, J.J.M. in 't Zand, and R.A.M.J. Wijers
One-dimensional Repulsive Fermi Gas in a Tunable Periodic Potential
Creators: name: Pilati, Sebastiano
name: Barbiero, Luca
name: Fazio, Rosario
name: Dell'Anna, Luca
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: By using unbiased continuos-space quantum Monte Carlo simulations, we investigate the ground state properties of a one-dimensional repulsive Fermi gas subjected to a commensurate periodic optical lattice (OL) of arbitrary intensity. The equation of state and the magnetic structure factor are determined as a function of the interaction strength and of the OL intensity. In the weak OL limit, Yang's theory for the energy of a homogeneous Fermi gas is recovered. In the opposite limit (deep OL), we analyze the convergence to the Lieb-Wu theory for the Hubbard model, comparing two approaches to map the continuous-space to the discrete-lattice model: the first is based on (noninteracting) Wannier functions, the second effectively takes into account strong-interaction effects within a parabolic approximation of the OL wells. We find that strong antiferromagnetic correlations emerge in deep OLs, and also in very shallow OLs if the interaction strength approaches the Tonks-Girardeau limit. In deep OLs we find quantitative agreement with density matrix renormalization group calculations for the Hubbard model. The spatial decay of the antiferromagnetic correlations is consistent with quasi long-range order even in shallow OLs, in agreement with previous theories for the half-filled Hubbard model.
description: 6 pages, 5 figures
Calpasoma dactylopterum Fuhrmann 1939
Creators: name: Calder, Dale R.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Limnomedusae
Olindiidae
Calpasoma
Calpasoma dactylopterum

description: Calpasoma dactylopterum Fuhrmann, 1939
Fig. 49
 Calpasoma dactyloptera Fuhrmann, 1939: 363, figs. 3–6.– Matthews, 1966: 256.
 Type locality. Switzerland: Neuchâtel, alongside Craspedacusta sowerbii in aquaria at the university (Fuhrmann 1939).
 Material examined. None.
 Description. (After Jankowski 2001): “Polyp…0.1–0.4 mm long; transparent to whitish; 8–32 (to 54) tentacles, 68–234 µm long and 8–15 µm wide; each tentacle contains 5–20 non grouped nematocyts (sic) (0.14 µm).”
 Remarks. Matthews (1966), working in Hawaii, reported Calpasoma dactylopterum Fuhrmann, 1939 on the aquatic tracheophyte Elodea canadensis, purchased from an unstated source. Specimens of this freshwater cnidarian were not represented in collections at the Bishop Museum, and it was not observed during this study.
 The cnidome of Calpasoma dactylopterum comprises heterotrichous microbasic euryteles, and reproduction occurs by formation of frustules (Rahat & Campbell 1974).
 There is disageement at present whether this is simply a form of Craspedacusta sowerbii Lankester, 1880.
 Reported distribution. Hawaii. Oahu: Honolulu, in aquaria on Elodea canadensis (Matthews 1966).
 Worldwide. Holarctic, shallow fresh waters (Jankowski et al. 2008).
description: Published as part of Calder, Dale R., 2010, Some anthoathecate hydroids and limnopolyps (Cnidaria, Hydrozoa) from the Hawaiian archipelago 2590, pp. 1-91 in Zootaxa 2590 (1) on page 75, DOI: 10.11646/zootaxa.2590.1.1, http://zenodo.org/record/10834110
Semiclassical approach to the decay of protons in circular motion under the influence of gravitational fields
Creators: name: Fregolente, Douglas
name: Matsas, George E. A.
name: Vanzella, Daniel A. T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the possible decay of protons in geodesic circular motion around neutral compact objects. Weak and strong decay rates and the associated emitted powers are calculated using a semi-classical approach. Our results are discussed with respect to distinct ones in the literature, which consider the decay of accelerated protons in electromagnetic fields. A number of consistency checks are presented along the paper.
description: To appear in Physical Review D
Additional file 5: of Overexpression of the protein disulfide isomerase AtCYO1 in chloroplasts slows dark-induced senescence in Arabidopsis
Creators: name: Tominaga, Jun
name: Nakahara, Yasutoshi
name: Horikawa, Daisuke
name: Tanaka, Ayumi
name: Kondo, Maki
name: Kamei, Yasuhiro
name: Takami, Tsuneaki
name: Sakamoto, Wataru
name: Unno, Kazutoshi
name: Sakamoto, Atsushi
name: Shimada, Hiroshi
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Plant Biology

description: Figure S2. Cotyledons at 9 DDI. (PDF 77Â kb)
Dirac particle dynamics of a superconducting circuit
Creators: name: Svetitsky, Elisha
name: Katz, Nadav
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The core concept of quantum simulation is the mapping of an inaccessible quantum system onto a controllable one by identifying analogous dynamics. We map the Dirac equation of relativistic quantum mechanics in 3+1 dimensions onto a multi-level superconducting Josephson circuit. Resonant drives determine the particle mass and momentum and the quantum state represents the internal spinor dynamics, which are cast in the language of multi-level quantum optics. The degeneracy of the Dirac spectrum corresponds to a degeneracy of bright/dark states within the system and particle spin and helicity are employed to interpret the multi-level dynamics. We simulate the Schwinger mechanism of electron-positron pair production by introducing an analogous electric field as a doubly degenerate Landau-Zener problem. All proposed measurements can be performed well within typical decoherence times. This work opens a new avenue for experimental study of the Dirac equation and provides a tool for control of complex dynamics in multi-level systems.
Forestry and woodworking skills in times of digital transformation
Creators: name: Kies, Uwe
Publisher: name: InnovaWood
Year: 2024

description: Overview of digital innovations in forestry, sawmilling, furniture, building with wood, and waste wood, and addresses the pros and cons of automation on jobs in the sector. It also provides a brief intro of the NEB Academy.

Presentation held at the EFBWW / ETUI workshop “Automation and technological change in woodworking and forestry”.
Decoherence in excited atoms by low-energy scattering
Creators: name: Quiñones, Diego A.
name: Varcoe, Benjamin
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We describe a new mechanism of decoherence in excited atoms as a result of thermal particles scattering by the atomic nucleus. It is based on the idea that a single scattering will produce a sudden displacement of the nucleus, which will be perceived by the electron in the atom as an instant shift in the electrostatic potential. This will leave the atom's wave-function partially projected into lower-energy states which will lead to decoherence of the atomic state. The decoherence is calculated to increase with the excitation of the atom, making observation of the effect easier in Rydberg atoms. We estimate the order of the decoherence for photons and massive particles scattering, analyzing several commonly presented scenarios. Our scheme can be applied to the detection of weakly-interacting particles, like those which may be the constituents of Dark Matter, which interaction was calculated to have a more prominent effect that the background radiation.
Euryglossula kubinensis Batley 2016, n. sp.
Creators: name: Batley, Michael
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Colletidae
Euryglossula
Euryglossula kubinensis

description: Euryglossula kubinensis n. sp.
Figs 11, 25, 34
 Type specimens. HOLOTYPE ♂, 5 km WSW of St Pauls, Moa (Banks) Is., Torres Strait, Queensland, 16 July 1977, G. Monteith and D. Cook, on Melaleuca, in QM (T234971). PARATYPES (14♀♀, all in QM), same data as holotype (QM T234972–985).
 Diagnosis. Female black or with faint metallic sheen, metasomal terga with conspicuously translucent apicolateral margins, tibiae and tarsi mostly yellow. Distinguished from E. incisa by convergent inner orbits and from E. elizabethae by tergal margins. Male face yellow to top of fovea, mandible with stiff setae ventrally, metasoma dark brown. Distinguished from E. aeneoceps by shorter fovea and from E. carnarvonensis by short lateral yellow marks on scutum.
 Description. Female.—Head width 0.93 mm, body length 3.3 mm. Relative measurements: HW 50, HL 41, UID 30, LID 25, FVL 11, CW 24, CL 7, FL 24. Head black or with faint metallic sheen, mandible yellow, antenna mottled yellow-brown. Frons weakly tessellate with close to dense punctures. Mesosoma black with the following yellow: tegula, alar sclerites, trochanters, femora apically, tibiae and tarsi (mid and hind tibiae with medial brown marks). Pronotal tubercle brown, wing veins weakly pigmented. Fore basitarsal setae stiff, weakly capitate; setae on ta2–4 stiff, apically hooked. Scutum weakly tessellate with dense punctures. Metasoma black, T2–5 with translucent margins, wider laterally. S3–5 apical margins translucent, preceded by narrow yellow line. Sculpture of frons, scutum, scutellum and dorsal surface of propodeum finely tessellate with fine, open punctures. Metasoma with transverse lineolation.
 Male.—Head width 0.80 mm, body length 2.5 mm. Relative measurements: HW 50, HL 43, UID 33, LID 25, FVL 6, CW 21, CL 8, FL 29. Head yellow with vertex, occiput and upper frons black. Mandible ventrally with ca 3 long, stiff setae. Frons and scutum dull with strong tessellation obscuring the weak punctures. Mesosoma black dorsally, except anterolateral corners of scutum yellow, just reaching anterior edge of tegula; ventrally yellow, except upper half mesepimeron and large spot on mesepisternum black. Metasoma brown dorsally, apical margins T2–6 translucent, ventrally yellow with irregular brown suffusions. Posterior margin S1 with rounded medial projection bearing plumose setae extending ½ length of S2. S5 with prominent apical fringe, long and uniform in length. Sculpture as for female.
 Etymology. The specific name refers to the collection location, currently known as Kubin Island.
description: Published as part of Batley, Michael, 2016, New Species of Euryglossula Michener (Apoidea: Colletidae), pp. 245-261 in Records of the Australian Museum 68 (6) on page 251, DOI: 10.3853/j.2201-4349.68.2016.1665, http://zenodo.org/record/10834437