cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Hamamelis virginiana gall versus leaf RNAseq scripts
Creators: name: Aishwarya Korgaonkar
name: Han, Clair
name: Stern, David
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Code used in analysis of Hamamelis virginiana gall versus leaf tissue RNAseq data, associated with the publication "A novel family of secreted insect proteins linked to plant gall development" by Korgaonkar et al. (2021).
Hvir_RNAseq_GallVsLeaf.sh: generates the RNAseq gene counts
GallVsLeafRNAseq_2020Sep_wUTR.R: plots figures 4G-H, S3D-E; (needs Gall-leaf-match-july2020.csv as input)

Please contact Clair Han at hanc@janelia.hhmi.org with questions.
Molecules, shocks, and disk in the axi-symmetric wind of the MS-type AGB star RS Cancri
Creators: name: Winters, J. M.
name: Hoai, D. T.
name: Wong, K. T.
name: Kim, W.
name: Nhung, P. T.
name: Tuan-Anh, P.
name: Lesaffre, P.
name: Darriulat, P.
name: Bertre, T. Le
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The latest evolutionary phases of low- and intermediate mass stars are characterized by complex physical processes like turbulence, convection, stellar pulsations, magnetic fields, condensation of solid particles, and the formation of massive outflows that inject freshly produced heavy elements and dust particles into the interstellar medium. We use the Northern Extended Millimeter Array (NOEMA) to obtain spatially and spectrally resolved observations of the semi-regular Asymptotic Giant Branch star RS Cancri to shed light on the morpho-kinematic structure of its inner, wind forming environment by applying detailed 3-D reconstruction modeling and LTE radiative transfer calculations. We detect 32 lines of 13 molecules and isotopologs (CO, SiO, SO, SO$_2$, H$_2$O, HCN, PN), including several transitions from vibrationally excited states. HCN, H$^{13}$CN, millimeter vibrationally excited H$_2$O, SO, $^{34}$SO, SO$_2$, and PN are detected for the first time in RS Cnc. Evidence for rotation is seen in HCN, SO, SO$_2$, and SiO(v=1). From CO and SiO channel maps, we find an inner, equatorial density enhancement, and a bipolar outflow structure with a mass loss rate of $1 \times 10^{-7}M_\odot{\rm yr}^{-1}$ for the equatorial region and of $2 \times 10^{-7}M_\odot{\rm yr}^{-1}$ for the polar outflows. The $^{12}$CO/$^{13}$CO ratio is measured to be $\sim20$ on average, $24\pm2$ in the polar outflows and $19\pm3$ in the equatorial region. We do not find direct evidence of a companion that might explain this kind of kinematic structure, and explore the possibility that a magnetic field might be the cause of it. The innermost molecular gas is influenced by stellar pulsation and possibly by convective cells that leave their imprint on broad wings of certain molecular lines, such as SiO and SO.
description: 28 pages, 40 figures, accepted for publication in Astronomy & Astrophysics
GÊNERO E JUSTIÇA ENERGÉTICA NA MINERAÇÃO DO CARVÃO EM SANTA CATARINA
Creators: name: Neiva, Sigrid de Aquino
name: Lampis, Andrea
name: Amaral., Daniela Higgin
name: Bermann, Celio
Publisher: name: figshare
Year: 2022
Subjects: Environmental Science

description: This study brings reflections of an exploratory research on the history of coal mining women in the state of Santa Catarina, as well as their possible relationship with the modern concept of energy justice and its guiding principles, in light of gender theories and feminist politics.
Hamamelis virginiana gall versus leaf RNAseq scripts
Creators: name: Aishwarya Korgaonkar
name: Han, Clair
name: Stern, David
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Code used in analysis of Hamamelis virginiana gall versus leaf tissue RNAseq data, associated with the publication "A novel family of secreted insect proteins linked to plant gall development" by Korgaonkar et al. (2021).
The Massive Soft Anomalous Dimension Matrix at Two Loops
Creators: name: Mitov, Alexander
name: Sterman, George
name: Sung, Ilmo
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study two-loop anomalous dimension matrices in QCD and related gauge theories for products of Wilson lines coupled at a point. We verify by an analysis in Euclidean space that the contributions to these matrices from diagrams that link three massive Wilson lines do not vanish in general. We show, however, that for two-to-two processes the two-loop anomalous dimension matrix is diagonal in the same color-exchange basis as the one-loop matrix for arbitrary masses at absolute threshold and for scattering at ninety degrees in the center of mass. This result is important for applications of threshold resummation in heavy quark production.
description: 7 pages, 3 figures, revtex
Understanding hydrogen permeation through molten metal alloy membranes
Creators: name: Byun, Dong Wook (Michael)
Publisher: name: University of British Columbia
Year: 2025

description: Selective separation of hydrogen has many potential benefits, but no existing hydrogen membranes can be operated at temperatures higher than 550 ºC without deactivation. Molten gallium and indium membranes have recently been reported to allow high temperature operation but the overall flux falls short of state-of-the-art palladium-based membranes due to slow dissociative adsorption of hydrogen. In order to increase the rate of dissociative adsorption, this thesis investigates molten alloy of transition metals with low melting metals for the first time. Five criteria were used to identify the candidate alloys for testing: vapour pressure, oxide and hydride stability, toxicity, state of matter, and material cost. Hydrogen dissociation on surfaces of molten metals and metal alloys was quantified using H₂-D₂ isotopic exchange reaction experiments in the temperature range of 450 – 650 ºC. Dissociative adsorption rates were higher for alloys: activation energies of hydrogen dissociation dropped from 187 kJ/mol for pure molten bismuth to 91 kJ/mol for molten Cu₀.₀₃Bi₀.₉₇. Hydrogen sorption into molten bismuth and bismuth alloys was quantified based using Sievert’s apparatus. Alloying copper and nickel to bismuth accelerated the sorption rate. Hydrogen sorption rates were determined to be between 7.10 × 10⁻⁵ mol/m²·s and 1.22 × 10⁻⁴ mol/m²·s, almost two orders of magnitudes slower than the rate of dissociative adsorption at 550 ºC. This indicated that diffusion was rate-limiting and the diffusion coefficients of 9.4 × 10⁻⁹ m²/s to 1.9 × 10⁻⁸ m²/s were calculated. Alloying transition metals with low melting metals increased the rate of dissociative adsorption without penalty to the rate of diffusion. Hydrogen permeation experiments in a small lab-scale membrane apparatus were challenged due to poor wetting of the top candidates identified on quartz. In order to investigate this, wetting of copper-bismuth alloys to porous substrates was evaluated. Non-reactive wetting of Cu₀.₀₃Bi₀.₉₇ and Cu₀.₀₃Sn₀.₉₇ to porous quartz substrate exhibited contact angles of 110º and 120º respectively. Reactive wetting of copper-bismuth alloys was also investigated by adding chromium which forms a chromium carbide layer on thin graphite, resulting in a decrease of contact angle from 90º to 45º.
The UKIRT Wide Field Camera ZYJHK Photometric System: Calibration from 2MASS
Creators: name: Hodgkin, S. T.
name: Irwin, M. J.
name: Hewett, P. C.
name: Warren, S. J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we describe the photometric calibration of data taken with the near-infrared Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope (UKIRT). The broadband ZYJHK data are directly calibrated from 2MASS point sources which are abundant in every WFCAM pointing. We perform an analysis of spatial systematics in the photometric calibration, both inter- and intra-detector and show that these are present at up to the 5 per cent level in WFCAM. Although the causes of these systematics are not yet fully understood, a method for their removal is developed and tested. Following application of the correction procedure the photometric calibration of WFCAM is found to be accurate to approximately 1.5 per cent for the JHK bands and 2 per cent for the ZY bands, meeting the survey requirements. We investigate the transformations between the 2MASS and WFCAM systems and find that the Z and Y calibration is sensitive to the effects of interstellar reddening for large values of E(B-V)', but that the JHK filters remain largely unaffected. We measure a small correction to the WFCAM Y-band photometry required to place WFCAM on a Vega system, and investigate WFCAM measurements of published standard stars from the list of UKIRT faint standards. Finally we present empirically determined throughput measurements for WFCAM.
description: Accepted on 2008 December 11 for publication in the MNRAS, 20 pages Remade Figure 11 which was corrupted during compression for astro-ph
Hamamelis virginiana red versus green gall RNAseq scripts
Creators: name: Aishwarya Korgaonkar
name: Han, Clair
name: Stern, David
Publisher: name: figshare
Year: 2020
Subjects: subject: Plant Biology
subject: FOS: Biological sciences

description: Code used in analysis of Hamamelis virginiana red gall tissue versus green gall tissue RNAseq data, associated with the publication "A novel family of secreted insect proteins linked to plant gall development" by Korgaonkar et al. (2021).
Hvir_RNAseq_RedVsGreen.sh: generates the RNAseq gene counts
RedVsGreenRNAseq_2020Sep_wUTR.R: plots figures 4A, S3B-C
RedVsGreenRNAseq_Counts_2020Sep_wUTR.R: plots figure 4B

Please contact Clair Han at hanc@janelia.hhmi.org with questions.
Effect of nonflow and flow fluctuations on elliptic flow methods
Creators: name: Ollitrault, Jean-Yves
name: Poskanzer, Arthur M.
name: Voloshin, Sergei A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We discuss how the different estimates of elliptic flow are influenced by flow fluctuations and nonflow effects. It is explained why the event-plane method yields estimates between the two-particle correlation methods and the multiparticle correlation methods. It is argued that nonflow effects and fluctuations cannot be disentangled without other assumptions. However, we provide equations where, with reasonable assumptions about fluctuations and nonflow, all measured values of elliptic flow converge to a unique mean elliptic flow in the participant plane. Thus, the 20% spread in observed elliptic flow measurements from different analysis methods is no longer mysterious.
description: For Quark Matter 2009 proceedings. Fig. 1 redrawn
title: Ð¢ÐµÑ Ð½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð² Ñ ÑÑÐµÑÐ¾Ð¼ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÐºÐ¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ»ÑÑÐ¸ÐºÐ¾Ð²Ð°, ÐÐ²Ð³ÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
ÑÐµÑ Ð½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÐºÐ¸

description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ Ð¢Ð­Ð ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð².
The P Cygni supergiant [OMN2000] LS1 - implications for the star formation history of W51
Creators: name: Clark, J. S.
name: Davies, B.
name: Najarro, F.
name: MacKenty, J.
name: Crowther, P. A.
name: Messineo, M.
name: Thompson, M. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigated the nature of the massive star [OMN2000] LS1 and used these results to constrain the history of star formation within the host complex W51. A combination of near-IR spectroscopy and non-LTE model atmosphere analysis was used to derive the physical properties of [OMN2000] LS1 and a combination of theoretical evolutionary calculations and Monte Carlo simulations to apply limits on the star formation history of W51. The spectrum of [OMN2000] LS1 is consistent with that of a P Cygni supergiant, but with a temperature of 13.2-13.7kK and log(L/L_sun)<5.75, it is significantly cooler, less luminous, and massive than proposed by previous authors. The presence of such a star within W51 shows that star formation has been underway for at least 3Myr, while the formation of massive O stars is still on going. We find no evidence of internally triggered, sequential star formation within W51, and favour the suggestion that star formation has proceeded at multiple indepedent sites within the GMC. [ABRIDGED]
description: 7 pages, 4 figures (Fig. 1 reduced in quality), accepted for publication in Astronomy and Astrophysics
Is it possible to construct excited-state energy functionals by splitting k-space?
Creators: name: Hemanadhan, M.
name: Harbola, Manoj K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: FOS: Physical sciences

description: We show that our procedure of constructing excited-state energy functionals by splitting k-space, employed so far to obtain exchange energies of excited-states, is quite general. We do so by applying the same method to construct modified Thomas-Fermi kinetic energy functional and its gradient expansion up to the second order for the excited-states. We show that the resulting kinetic energy functional has the same accuracy for the excited-states as the ground-state functionals do for the ground-states.
description: 20 pages, 1 figure
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ°Ð²Ð¸Ð» Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ GPU
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð»ÑÑÐµÐ², ÐÐ»ÐµÐ±
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ
ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ·ÑÐºÐ¸
ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¸Ð»Ð°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ°Ð²Ð¸Ð». Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ°Ð²Ð¸Ð». Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¼Ð¾Ð´Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Eclat Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ CN2 Ð½Ð° CPU Ð¸ GPU. ÐÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¸ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ.
New Completeness Methods for Estimating Exoplanet Discoveries by Direct Detection
Creators: name: Brown, Robert A.
name: Soummer, Remi
Publisher: name: arXiv
Year: 2010
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report new methods for evaluating realistic observing programs that search stars for planets by direct imaging, where observations are selected from an optimized star list, and where stars can be observed multiple times. We show how these methods bring critical insight into the design of the mission & its instruments. These methods provide an estimate of the outcome of the observing program: the probability distribution of discoveries (detection and/or characterization), & an estimate of the occurrence rate of planets (eta). We show that these parameters can be accurately estimated from a single mission simulation, without the need for a complete Monte Carlo mission simulation, & we prove the accuracy of this new approach. Our methods provide the tools to define a mission for a particular science goal, for example defined by the expected number of discoveries and its confidence level. We detail how an optimized star list can be built & how successive observations can be selected. Our approach also provides other critical mission attributes, such as the number of stars expected to be searched, & the probability of zero discoveries. Because these attributes depend strongly on the mission scale, our methods are directly applicable to the design of such future missions & provide guidance to the mission & instrument design based on scientific performance. We illustrate our new methods with practical calculations & exploratory design reference missions for JWST operating with a distant starshade to reduce scattered and diffracted starlight on the focal plane. We estimate that 5 habitable Earth-mass planets would be discovered & characterized with spectroscopy, with a probability of 0 discoveries of 0.004, assuming a small fraction of JWST observing time (7%), eta=0.3, and 70 observing visits, limited by starshade fuel.
description: 27 pages, 4 figures, 6 tables, accepted for publication by ApJ
Additional file 3 of A novel inflammatory response-related signature predicts the prognosis of cutaneous melanoma and the effect of antitumor drugs
Creators: name: Xing, Jiahua
name: Li, Yan
name: Chen, Youbai
name: Han, Yan
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Mental Health

description: Additional file 3.
title: ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ³ÑÐ½Ð¾Ð², ÐÑÑÐµÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ
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description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¼Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ² Ð¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹. ÐÑÑÐ»ÐµÐ´ÑÑÑÑÑ ÑÑÑÐ½Ð¾ÑÑÑ Ð¸ Ð²Ð¸Ð´Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ð¹ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ. Ð ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ Ð´Ð¾Ð³Ð¾Ð²Ð¾ÑÑ Ð¸ ÐºÐ¾Ð½Ð²ÐµÐ½ÑÐ¸Ð¸ Ð² ÑÑÐµÑÐµ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð°. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð°ÐºÑÑ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸, Ð¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð°ÐºÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼ÐµÑÑ, ÑÐµÐ»ÑÑ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð±Ð¾ÑÑÐ±Ð° Ð¸ Ð¿ÑÐµÐ´ÑÐ¿ÑÐµÐ¶Ð´ÐµÐ½Ð¸Ðµ Ð½Ð°Ð½ÐµÑÐµÐ½Ð¸Ñ ÑÑÐµÑÐ±Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ðµ, Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°. ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¾Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð° Ð¸ Ð¸Ñ ÑÐ¾Ð»Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. ÐÑÑÐ²Ð»ÑÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð¾ÑÑÐ°Ð½Ñ Ð²Ð¾Ð´ Ð¾Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ. ÐÐ·ÑÑÐ°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð¾ÑÑÐ°Ð½Ñ Ð°ÑÐ¼Ð¾ÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÑÑÐ° Ð¾Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ.
Kinematic Signatures of Subvirial Initial Conditions in Young Clusters
Creators: name: Proszkow, Eva-Marie
name: Adams, Fred C.
name: Hartmann, Lee W.
name: Tobin, John J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Motivated by kinematic observations of young embedded clusters, this paper explores possible kinematic signatures produced by asphericity and departures from initial virial equilibrium in these systems. Specifically, the kinematic quantity that is measured and calculated in this study is the distribution of the line-of-sight velocities as a function of position along the cluster. Although clusters are found within a wide range of sizes, we focus on the regime with stellar membership $N \sim 10^3$. The gravitational potential of these young clusters is dominated by the gas, and the geometry of the gas distribution is generalized to include axisymmetric (and triaxial) forms. With this loss of symmetry, the kinematic results thus depend on viewing angle. This work also considers the stars to begin their trajectories with subvirial speeds, as indicated by observations of core motions in such clusters. Our results determine the conditions necessary for the kinematic signature to display interesting structure, i.e., a non-spherical potential, a viewing angle that is not along one of the principal axes, and subvirial starting conditions. We characterize the effects on this signature due to projection angle, initial stellar velocities, cluster elongation, and star formation efficiency. Finally, we compare our theoretical results to recent kinematic observations of the Orion Nebula Cluster; we find that the observations can be explained provided that the cluster is non-spherical, starts with subvirial initial velocities, and is not viewed along a principal axis.
description: 13 pages, 10 figures, Accepted for publication in ApJ
Characterization of autosomal dominant retinitis pigmentosa-associated rhodopsin missense mutations in Xenopus laevis rod photoreceptors
Creators: name: Loewen, Aaron Daniel
Publisher: name: University of British Columbia
Year: 2025

description: Retinitis pigmentosa (RP) is an inherited retinal disease that causes progressive vision loss due to retinal degeneration. RP has at least three associated clinical classes, each with differing disease presentations in patients. One subclass is sector RP, which is less severe than typical RP and has only one or two affected retinal quadrants. Due to the asymmetric phenotype, sector RP is hypothesized to be exacerbated by light exposure. Over a third of autosomal dominant RP (adRP) cases are associated with mutations in rhodopsin (RHO), which encodes the visual pigment in rod photoreceptors. Over 200 mutations have been identified as pathogenic; however, the pathogenic mechanisms associated with most mutations is unknown. Well-studied mutations include P23H RHO, which causes misfolding of RHO and undergoes ER stress-related cell death, and T4K RHO, which is partially glycosylation-deficient and causes a photoactivation-induced toxicity mechanism. These mutations cause the same disease but have contrasting characteristics regarding pathogenic mechanisms, highlighting the potential variability of cellular consequences in RHO-associated adRP. In this thesis, I aimed to characterize uncharacterized RHO mutations and their associated pathogenic mechanisms by generating transgenic Xenopus laevis models of RP. We identified and described a novel RHO mutation associated with sector RP and created an experimental paradigm to characterize mutations in vivo. This was applied to another 26 uncharacterized mutations, where we evaluated RHO localization, retinal degeneration, RHO glycosylation, and effects of photoactivation on retinal degeneration. The majority of the mutations investigated caused retinal degeneration in our models. We further identified that all but two mutations (P23H and S176F) are predominantly trafficked to the rod outer segment. Several sector RP-associated mutations caused light-dependent degeneration, which aligns with published data; however, we identified a group of sector RP mutations that caused light-independent degeneration and abnormal RHO multimerization. Overall, we propose new classifications of RHO mutations based on pathogenic mechanisms described in vivo. We identified a set of sector RP-associated mutations that activate novel pathogenic mechanisms. A variety of mechanisms should be considered when developing and evaluating RHO-associated RP treatment options.
Galaxy populations in the Hydra I cluster from the VEGAS survey I. Optical properties of a large sample of dwarf galaxies
Creators: name: La Marca, Antonio
name: Peletier, Reynier
name: Iodice, Enrichetta
name: Paolillo, Maurizio
name: Challapa, Nelvy Choque
name: Venhola, Aku
name: Forbes, Duncan A.
name: Cantiello, Michele
name: Hilker, Michael
name: Rejkuba, Marina
name: Arnaboldi, Magda
name: Spavone, Marilena
name: D'Ago, Giuseppe
name: Raj, Maria Angela
name: Ragusa, Rossella
name: Mirabile, Marco
name: Rampazzo, Roberto
name: Spiniello, Chiara
name: Mieske, Steffen
name: Schipani, Pietro
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: At ~50 Mpc, the Hydra I cluster of galaxies is among the closest cluster in the z=0 Universe, and an ideal environment to study dwarf galaxy properties in a cluster environment. We exploit deep imaging data of the Hydra I cluster to construct a new photometric catalog of dwarf galaxies in the cluster core, which is then used to derive properties of the Hydra I cluster dwarf galaxies population as well as to compare with other clusters. Moreover, we investigate the dependency of dwarf galaxy properties on their surrounding environment. The new Hydra I dwarf catalog contains 317 galaxies with luminosity between -18.5
description: Accepted for publication in A&A. 25 pages, 21 figures
CADASTROS TÉCNICOS FEDERAIS: INSTRUMENTOS DA POLÍTICA AMBIENTAL
Creators: name: Vianna, Simone de Castro
name: Agra, Roberto Martins
Publisher: name: figshare
Year: 2022
Subjects: Environmental Science

description: This study describes the Federal Technical Register of Activities and Instruments of Environmental Defense (CTF/AIDA) and the Federal Technical Register of Potentially Polluting Activities and Users of Environmental Resources (CTF/APP), instruments of the National Environmental Act (PNMA), under Ibama management. Created under different circumstances, the registers poses different characteristics regarding their purposes and the public that are subjected to registration. The CTF/AIDA is for disclosure of specific environmental compentences and the CTF/APP aims to gather information and data for environmental management at the national level. The regulation historical background revealed the predominance of a unified perspective of both registers, under the name of “Federal Technical Registry”, in disagreement with the normative definition itself. In addition, the alternation between Ibama's managing areas gave the registers characteristics of control of polluting activities or taxation, distorting the purpose for which they were created. In 2006, a regulation improvement began by the Environmental Quality Board, despite the maintenance of a single system of registers. In 2013, the definitive segregation of the registers accompanied with publication of new regulation and the development of independent systems, once again consolidated the individualization of both instruments. This separation is a requirement for transparency and essential for evaluating the registers. These findings are expected to contribute to the debate on PNMA instruments and the generation of environmental information, through studies that seek to analyze the effectiveness of the registers, evaluate the applicability of other associated mechanisms, integration with other instruments and operationalization of SISNAMA.
Additional file 1 of Super-enhancer hijacking LINC01977 promotes malignancy of early-stage lung adenocarcinoma addicted to the canonical TGF-β/SMAD3 pathway
Creators: name: Zhang, Te
name: Xia, Wenjie
name: Song, Xuming
name: Mao, Qixing
name: Huang, Xing
name: Chen, Bing
name: Liang, Yingkuan
name: Wang, Hui
name: Chen, Yuzhong
name: Yu, Xinnian
name: Zhang, Zeyu
name: Yang, Wenmin
name: Xu, Lin
name: Dong, Gaochao
name: Jiang, Feng
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Science Policy
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Supplementary Figures.
title: Ð£ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ ÑÐ³ÑÐ¾Ð·Ðµ ÑÐµÑÑÐ¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°ÐºÑÐ¾Ð² Ð½Ð° Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½ÑÑ ÑÑÐ°Ð½ÑÐ¸ÑÑ Ð¸ Ð²Ð¾ÐºÐ·Ð°Ð»Ð°Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¼Ð¸Ð½Ð¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÑÑÐ¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°ÐºÑ
Ð²Ð·ÑÑÐ²ÑÐ°ÑÐ¾Ðµ Ð²ÐµÑÐµÑÑÐ²Ð¾
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description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐµÑÑÐ¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð°ÐºÑÐ°Ð¼ Ð² Ð Ð¾ÑÑÐ¸Ð¸. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½ ÑÐµÑÑÐ¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°ÐºÑ Ð² Ð³Ð¾ÑÐ¾Ð´Ðµ ÐÐµÑÐ±ÐµÐ½Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ°Ñ Ð°Ð½ÑÐ¸ÑÐµÑÑÐ¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÑÑ Ð·Ð°ÑÐ¸ÑÑ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¸Ð¼ÐµÑÑÐµÐ¹ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾ÑÐ°Ñ Ð³Ð»Ð°Ð²Ð° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½ÑÑ ÑÑÐ°Ð½ÑÐ¸ÑÑ Ð¸ Ð²Ð¾ÐºÐ·Ð°Ð»Ð°Ñ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð¾ÑÐ¼ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð½ÑÑ Ð½ÐµÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ². Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¾Ð±ÑÐµÐºÑÐ° Ð¾ÑÑÐ°Ð½Ñ (Ð²Ð¾ÐºÐ·Ð°Ð»Ð° Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐµÑÐ±ÐµÐ½Ñ) Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸ÐµÐ¼ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°. Ð Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ð¸ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¸ Ð¿Ð¾Ð´Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÐ¾Ð³Ð¸ ÑÐ°Ð±Ð¾ÑÑ.
title: Rapport annuel et bilan social/Loterie romande
title: Rapport annuel et bilan social/Loterie romande
titleType: AlternativeTitle
Creators: name: Société De La Loterie De La Suisse Romande (LoRo)
Publisher: name: Loterie Romande
Year: 2010

description: Légère variation du titre pour 2010 : Rapport annuel, bilan social/Loterie romande
Additional file 1 of Atmospheric resuspension of insoluble radioactive cesium-bearing particles found in the difficult-to-return area in Fukushima
Creators: name: Tang, Peng
name: Kita, Kazuyuki
name: Igarashi, Yasuhito
name: Satou, Yukihiko
name: Hatanaka, Koutarou
name: Adachi, Kouji
name: Kinase, Takeshi
name: Ninomiya, Kazuhiko
name: Shinohara, Atsushi
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences

description: Additional file 1. Supporting figures and tables.
AS CONDIÇÕES DE TRABALHO DE CATADORES DE MATERIAIS RECICLÁVEIS DURANTE A PANDEMIA DE COVID-19 EM BELÉM-PA
Creators: name: Santana, João Victor
Publisher: name: figshare
Year: 2022
Subjects: Environmental Science

description: In March 2020, the World Health Organization declared the Covid-19 pandemic. With the increase in the number of deaths due to the virus and social isolation, the population began to present physical and mental health problems. In this scenario, the importance of health care measures for workers and the population in general is highlighted, aiming at mitigating the negative impacts caused by the pandemic. The present work sought to carry out an analysis of the circumstances and working conditions faced by recyclable material collectors during the Covid-19 pandemic in the municipality of Belém - PA. The survey was carried out in January 2021, and interviewers who were working at that time were interviewed. The interview took place through the application of a checklist and a questionnaire. Thus, it is considered that the present work is a field research, with a descriptive and exploratory character and having its construction done through bibliographic and documentary research. It was observed that the equipment used by these workers during their activities does not qualify as PPE and that the most significant change for this period was the use of handmade fabric masks. The actions developed by the associations and cooperatives to which the interviewees are linked, proved to be valid in relation to the pandemic context. Thus, there is a need for actions that promote awareness of the use of PPE by this working class, as well as the appreciation of these institutions that are so important in the lives of these workers.
title: Useful words and facts. Ð¢ÐµÐºÑÑÐ¾Ð²ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÐ»Ð¾Ð²Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ»Ð¾Ð²Ð¾ÑÐ¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ñ. Ð§. 1
title: ÐºÐ»ÑÑÐ¸ Ðº ÑÑÐµÐ±Ð½Ð¾Ð¼Ñ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¼Ð°ÑÐ¸Ð½Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: ÐÐµÐ»ÑÐµÐ²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÑÐ»Ð¾Ð²Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ»Ð¾Ð²Ð¾ÑÐ¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ðµ
Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ²ÑÐ¾ÑÑ Ð½Ð°Ð¼ÐµÑÐµÐ½Ð½Ð¾ Ð²ÑÐ¿ÑÑÑÐ¸Ð»Ð¸ ÐºÐ»ÑÑÐ¸ Ðº Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð² Ð²Ð¸Ð´Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ, Ñ.Ðº., Ð¿Ð¾ Ð¸Ñ Ð¼Ð½ÐµÐ½Ð¸Ñ, Ð¾ÑÑÑÑÑÑÐ²Ð¸Ðµ Ð¿Ð¾Ð´ÑÐºÐ°Ð·ÐºÐ¸ Ð² ÑÐ°Ð¼Ð¾Ð¼ ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð´Ð¾Ð»Ð¶Ð½Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²Ð¾Ð²Ð°ÑÑ, Ñ ÑÑÐ°ÑÐ¸ÑÑÑ Ð²ÑÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ¼ÐµÐ½Ð¸Ð¹ ÑÐµÑÐ°ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð°ÑÑÐ¸ÑÑ Ð¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼Ð¸ Ð²Ð¸Ð´Ð°Ð¼Ð¸ ÑÐ»Ð¾Ð²Ð°ÑÐµÐ¹ Ð¸ Ð´ÑÑÐ³Ð¾Ð¹ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ¾Ð¹.
E-Leaning System for Using The Morphological Matrix Method in the Technical Creation
Creators: name: Neculai-Eugen, Seghedin; Dragos, Chitariu
Publisher: name: Editura Universitara
Year: 2012
Subjects: subject: 0 Social sciences
subject: 37 Education
subject: 371 Instructional design
subject: 004:37 Elearning

description: In technical creation domain, there are a lot of methods and techniques that can be used for stimulation of technical creativity. These methods and techniques can be divided into two main categories: the psychological creativity methods and the logical (logical-combinatorial) creativity methods. These two types of methods are both used, but the key of success is the alternative use of them. The morphological matrix method consists on the logical combination of elements from a technical system. This way, it is possible to obtain new technical solutions, according to the combination generated.
A possible solution to the Milky Way's binary-deficient retrograde stellar population. Evidence that $ω$ Centauri has formed in an extreme starburst
Creators: name: Marks, M.
name: Kroupa, P.
name: Dabringhausen, J.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. The fraction of field binaries on retrograde orbits about the Milky Way is significantly lower compared to its prograde counterpart. Chemical and dynamical evidence suggests that the retrograde stellar population originates from $ω$ Centauri, which is either the most massive globular cluster (GC) of the Milky Way or the putative core of a former dwarf galaxy. Aims. Star formation conditions required to produce the retrograde binary population are constrained assuming that the retrograde stellar population originates from $ω$ Centauri's progenitor. Methods. We match the observed low binary fraction with dynamical population synthesis models, including a universal initial binary population and dynamical processing in star clusters, making use of the publicly available binary population synthesis tool BiPoS1. Results. It is found that either the GC progenitor of $ω$ Centauri must have formed with a stellar density of $\approx 10^8 \; M_{sun} \; pc^{-3}$ or the $ω$ Centauri dwarf galaxy's progenitor star cluster population must have formed in an extreme starburst with a star formation rate exceeding $1000 \; M_{sun} \; yr^{-1}$ and probably a top-heavy embedded-cluster mass function with suppressed low-mass cluster formation. The separation and mass ratio distribution for retrograde field binaries are predicted for comparison with future observations. Conclusions. A viable solution for the deficiency of binaries on retrograde orbits is presented, and star formation conditions for $ω$ Centauri as well as orbital parameter distributions for the Milky Way's retrograde binary population are predicted. The dwarf galaxy origin for $ω$ Centauri is tentatively preferred within the present context.
description: accepted for publication in A&A, 9 pages, 3 figures
Additional file 3: of Bloodstream infections caused by Klebsiella pneumoniae: prevalence of blaKPC, virulence factors and their impacts on clinical outcome
Creators: name: Xu, Min
name: Fu, Yiqi
name: Kong, Haishen
name: Chen, Xiao
name: Chen, Yu
name: Li, Lanjuan
name: Yang, Qing
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Figure S1. Characteristics of 54Â K. pneumoniae isolates from the non-survival subgroup. (PDF 1596 kb)
Rest-frame ultraviolet spectrum of the gravitationally lensed galaxy `the 8 o'clock arc': stellar and interstellar medium properties
Creators: name: Dessauges-Zavadsky, M.
name: D'Odorico, S.
name: Schaerer, D.
name: Modigliani, A.
name: Tapken, C.
name: Vernet, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the first detailed analysis of the rest-frame UV spectrum of the gravitationally lensed Lyman break galaxy (LBG), the `8 o'clock arc'. The spectrum of the 8 o'clock arc is rich in stellar and interstellar medium (ISM) features, and presents several similarities to the well-known MS1512-cB58 LBG. The stellar photospheric absorption lines allowed us to constrain the systemic redshift, z_sys = 2.7350+/-0.0003, of the galaxy, and derive its stellar metallicity, Z=0.82 Z_sol. With a total stellar mass of ~4.2x10^{11} M_sol, the 8 o'clock arc agrees with the mass-metallicity relation found for z>2 star-forming galaxies. The 31 ISM absorption lines detected led to the abundance measurements of 9 elements. The metallicity of the ISM, Z=0.65 Z_sol (Si), is very comparable to the metallicity of stars and ionized gas, and suggests that the ISM of the 8 o'clock arc has been rapidly polluted and enriched by ejecta of OB stars. The ISM lines extend over ~1000 km/s and have their peak optical depth blueshifted relative to the stars, implying gas outflows of about -120 km/s. The Ly-alpha line is dominated by a damped absorption profile on top of which is superposed a weak emission, redshifted relative to the ISM lines by about +690 km/s and resulting from multiply backscattered Ly-alpha photons emitted in the HII region surrounded by the cold, expanding ISM shell. A homogeneous spherical radiation transfer shell model with a constant outflow velocity, determined by the observations, is able to reproduce the observed Ly-alpha line profile and dust content. These results fully support the scenario proposed earlier, where the diversity of Ly-alpha line profiles in LBGs and Ly-alpha emitters, from absorption to emission, is mostly due to variations of HI column density and dust content (abridged).
description: 17 pages, 10 figures, A&A, accepted
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ "Ð ÑÑÐ°Ð³ Ñ Ð³Ð¾Ð»Ð¾Ð²ÐºÐ°Ð¼Ð¸, Ð»ÐµÐ¶Ð°ÑÐ¸Ð¼Ð¸ Ð² ÑÐ°Ð·Ð½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐºÐ¾ÑÑÐ¸"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð³ÑÐ½Ð±ÐµÐºÐ¾Ð², ÐÑÑÐ°Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
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description: ÐÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐµÐ¹ ÑÐ²Ð»ÑÐµÑÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ. Ð ÑÐ°ÐºÐ¸Ð¼ Ð·Ð°Ð´Ð°ÑÐ°Ð¼ Ð¾ÑÐ½Ð¾ÑÑÑÑÑ: ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð², Ð´Ð¾Ð¿ÑÑÐºÐ¸ ÑÐ¾ÑÐ¼Ñ, Ð´Ð¾Ð¿ÑÑÐºÐ¸ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¸ Ð¼ÐµÑÑÐ¾ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, Ð´Ð¾Ð¿ÑÑÐºÐ¸ Ð±Ð¸ÐµÐ½Ð¸Ð¹, ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð³Ð¾ ÑÐ»Ð¾Ñ, ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°. Ð Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ»ÑÑÐ°ÑÑ Ð¿ÑÐ¸ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°. Ð ÑÐ°ÐºÐ¸Ð¼ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð¼ Ð¾ÑÐ½Ð¾ÑÑÑÑÑ ÑÐ°ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÐ·ÑÑ, Ð¼ÐµÑÑÐ¸ÐºÐ¸, ÑÐµÑÐ²ÑÑÐ½ÑÐµ ÑÑÐµÐ·Ñ Ð¸ Ñ. Ð´. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð´Ð°Ð½Ð½ÑÑ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð¿Ð¾Ð²ÑÑÐ°ÐµÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐµÑÐ¸Ð¹Ð½Ð¾Ð³Ð¾ Ð¸ Ð¼Ð°ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ², ÐºÐ¾Ð³Ð´Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑ ÑÐµÑÐ°ÑÑÐµÐµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ, Ð¸Ð¼ÐµÐµÑ Ð¼ÐµÑÑÐ¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¾ÑÐ´ÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸ Ð¸Ð»Ð¸ Ð²ÑÐµÐ³Ð¾ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. ÐÐ»Ñ ÑÑÐ¸Ñ ÑÐµÐ»ÐµÐ¹ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÑÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾-ÑÐ°Ð·Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐµÐµ Ð²ÑÐµ ÑÐ°Ð±Ð¾ÑÐ¸Ðµ Ð¸ ÑÐ¾Ð»Ð¾ÑÑÑÐµ ÑÐ¾Ð´Ñ, Ð¿Ð¾Ð´Ð°ÑÑ, ÑÑÑÐ°Ð½Ð¾Ð²ÐºÑ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð² Ð·Ð°Ð¶Ð¸Ð¼Ð½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ Ð¸ Ð¾ÑÐ²Ð¾Ð´ Ð¿ÑÐ¸ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¼ Ð¸Ð»Ð¸ Ð±ÐµÐ· Ð½ÐµÐ¿Ð¾ÑÑÐµÐ´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐ¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°.
Collapse Barriers and Halo Abundance: Testing the Excursion Set Ansatz
Creators: name: Robertson, Brant
name: Kravtsov, Andrey
name: Tinker, Jeremy
name: Zentner, Andrew
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Our heuristic understanding of the abundance of dark matter halos centers around the concept of a density threshold, or "barrier", for gravitational collapse. If one adopts the ansatz that regions of the linearly evolved density field smoothed on mass scale M with an overdensity that exceeds the barrier will undergo gravitational collapse into halos of mass M, the corresponding abundance of such halos can be estimated simply as a fraction of the mass density satisfying the collapse criterion divided by the mass M. The key ingredient of this ansatz is therefore the functional form of the collapse barrier as a function of mass M or, equivalently, of the variance sigma^2(M). Several such barriers based on the spherical, Zel'dovich, and ellipsoidal collapse models have been extensively discussed. Using large scale cosmological simulations, we show that the relation between the linear overdensity and the mass variance for regions that collapse to form halos by the present epoch resembles expectations from dynamical models of ellipsoidal collapse. However, we also show that using such a collapse barrier with the excursion set ansatz predicts a halo mass function inconsistent with that measured directly in cosmological simulations. This inconsistency demonstrates a failure of the excursion set ansatz as a physical model for halo collapse. We discuss implications of our results for understanding the collapse epoch for halos as a function of mass, and avenues for improving consistency between analytical models for the collapse epoch and the results of cosmological simulations.
description: Version accepted by ApJ, scheduled for May 2009, v696. High-res version available at http://kicp.uchicago.edu/~brant/astro-ph/excursion_set_ansatz/robertson_excursion_set_ansatz.pdf
Additional file 1 of The RXFP2-PLC/PKC signaling pathway mediates INSL3-induced regulation of the proliferation, migration and apoptosis of mouse gubernacular cells
Creators: name: Duan, Shouxing
name: Jiang, Xuewu
name: Li, Jianhong
name: Fu, Maxian
name: Li, Zhuo
name: Cheng, Yiyi
name: Zhuang, Yangmu
name: Yang, Ming
name: Xiao, Wenfeng
name: Ping, Hongyan
name: Xie, Yao
name: Xie, Xiaojun
name: Zhang, Xuan
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Figure S1. A schematic diagram to illustrate the experimental system for function confirmation of INSL3 regulating gubernacular cells and signaling pathways analysis.