cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
An Accurate Position for HDF 850.1: The Brightest Submillimeter Source in the Hubble Deep Field-North
Creators: name: Cowie, L. L.
name: Barger, A. J.
name: Wang, W. -H.
name: Williams, J. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report a highly significant Submillimeter Array (SMA) detection of the prototypical submillimeter source HDF 850.1, which is the brightest submillimeter source in the Hubble Deep Field-North proper. The detection yields an extremely precise position of RA(2000)=12:36:51.99 and Dec(2000)=+62:12:25.83 with a 1-sigma positional uncertainty of 0.17 arcsec. The position is consistent with the location of a millimeter wavelength interferometric detection and with the locations of weak VLA detections at 1.4 and 8.4 GHz, but it is not consistent with any previous optical/near-infrared identifications. The source appears pointlike at the 2 arcsec resolution of the SMA, and the detected flux of 7.8+/-1.0 mJy is consistent with the measured SCUBA fluxes. We tabulate fluxes and limits on HDF 850.1 at other wavelengths. Our redshift estimate for HDF 850.1 based on the radio through mid-infrared measurements is z=4.1. The faintness of the source at optical/near-infrared wavelengths and the high estimated redshift suggest that HDF 850.1 may be an analog of the brighter submillimeter source GOODS 850-5, which is also thought to be at z>4. The fact that a source like HDF 850.1 should have appeared in one of the very first blank-field SCUBA observations ever made suggests that such high-redshift sources are quite common. Thus, we are led to conclude that high-redshift star formation is dominated by giant dusty star-forming galaxies, just as it is at lower redshifts.
description: 5 pages
Response of Seven Crystallographic Orientations of Sapphire Crystals to Shock Stresses of 16 to 86 GPa
Creators: name: Kanel, G. I.
name: Nellis, W. J.
name: Savinykh, A. S.
name: Razorenov, S. V.
name: Rajendran, A. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Shock-wave profiles of sapphire (single-crystal Al2O3) with seven crystallographic orientations were measured with time-resolved VISAR interferometry at shock stresses in the range 16 to 86 GPa. Shock propagation was normal to the surface of each cut. The angle between the c-axis of the hexagonal crystal structure and the direction of shock propagation varied from 0 for c-cut up to 90 degrees for m-cut in the basal plane. Based on published shock-induced transparencies, shock-induced optical transparency correlates with the smoothness of the shock-wave profile. The ultimate goal was to find the direction of shock propagation in sapphire that is most transparent as a window. Particle velocity histories were recorded at the interface between a sapphire crystal and a LiF window. In most cases measured wave profiles are noisy as a result of heterogeneity of deformation. Measured values of Hugoniot Elastic Limits (HELs) depend on direction of shock compression and peak shock stress. The largest HEL values were recorded for shock loading along the c-axis and perpendicular to c along the m-direction. Shock compression along the m- and s-directions is accompanied by the smallest heterogeneity of deformation and the smallest rise time of the plastic shock wave. m- and s-cut sapphire most closely approach ideal elastic-plastic flow, which suggests that m- and s-cut sapphire are probably the orientations that remains most transparent to highest shock pressures. Under purely elastic deformation sapphire has very high spall strength, which depends on load duration and peak stress. Plastic deformation of sapphire causes loss of its tensile strength.
description: 18 pages, 18 figures
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÐºÐ¾Ð»ÑÑÐµÐ²ÑÑ ÑÐµÐ·Ð¾Ð½Ð°ÑÐ¾ÑÐ¾Ð² Ð±ÐµÐ³ÑÑÐµÐ¹ Ð²Ð¾Ð»Ð½Ñ Ð½Ð° Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð°ÑÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·Ð»ÑÑÐ°ÑÐµÐ»Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾ÐºÐ¾Ð¿ÑÑÐº, Ð Ð¾Ð¼Ð°Ð½
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: ÐºÐ¾Ð»ÑÑÐµÐ²ÑÐµ ÑÐµÐ·Ð¾Ð½Ð°ÑÐ¾ÑÑ
Ð±ÐµÐ³ÑÑÐ°Ñ Ð²Ð¾Ð»Ð½Ð°
Ð¿Ð°ÑÑÐ¸Ð°Ð»ÑÐ½ÑÐ¹ Ð¸Ð·Ð»ÑÑÐ°ÑÐµÐ»Ñ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, ÑÐµÑÑÑÑÑ Ð³Ð»Ð°Ð² Ð¸ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ. ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÐºÑÐ°ÑÐºÐ¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð° ÑÐ¾Ð»Ñ ÑÐµÐ·Ð¾Ð½Ð°ÑÐ¾ÑÐ¾Ð² Ð±ÐµÐ³ÑÑÐµÐ¹ Ð²Ð¾Ð»Ð½Ñ (Ð ÐÐ) Ð² ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐµ, ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÑÐµÐ±ÑÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ°ÑÑÑÑ Ð¿Ð¾Ð»Ñ Ð½Ð° Ð¾Ð´Ð¸Ð½Ð¾ÑÐ½Ð¾Ð¼ ÐºÐ¾Ð»ÑÑÐµ, Ð²Ð·ÑÑÑÐ¹ Ð¸Ð· Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð¿Ð¾ÑÐºÐ¾Ð»ÑÐºÑ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð²Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¸ ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ð°Ñ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ñ Ð½Ð° ÑÑÐ¾Ð¼ ÑÐ°ÑÑÑÑÐµ. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð¿Ð¾Ð»Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÐºÐ¾Ð»ÑÑÐ° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ ÐºÐ¾Ð»ÑÑÐ°. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½ ÑÐ¾Ðº Ð½Ð° Ð²Ð½ÐµÑÐ½ÐµÐ¼ ÐºÐ¾Ð»ÑÑÐµ. Ð ÑÐµÑÐ²ÑÑÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð½Ð°Ð¹Ð´ÐµÐ½Ð° Ð½ÐµÐ¿Ð¾ÑÑÐµÐ´ÑÑÐ²ÐµÐ½Ð½Ð¾ Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ð° Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸Ð·Ð»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð². Ð Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ð¸ ÑÐ´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¿Ð¾ Ð¸ÑÐ¾Ð³Ð°Ð¼ ÑÐ°ÑÑÑÑÐ¾Ð².
A_N in inclusive lepton-proton collisions
Creators: name: M. Anselmino
name: M. Boglione
name: U. D'Alesio
name: S. Melis
name: F. Murgia
name: A. Prokudin
Publisher: name: INFN Open Access Repository
Year: 2014

description: Some estimates for the transverse single spin asymmetry, A_N, in the
inclusive processes l p(transv. pol.) -> h X are compared with new experimental
data. The calculations are based on the Sivers and Collins functions as
extracted from SIDIS azimuthal asymmetries, within a transverse momentum
dependent factorization approach. The values of A_N thus obtained agree in sign
and shape with the data. Predictions for future experiments are also given.
CMB quenching of high-redshift radio-loud AGNs
Creators: name: G. Ghisellini
name: F. Haardt
name: B. Ciardi
name: T. Sbarrato
name: E. Gallo
name: F. Tavecchio
name: A. Celotti
Publisher: name: INFN Open Access Repository
Year: 2015

description: The very existence of more than a dozen of high-redshift (z>4) blazars
indicates that a much larger population of misaligned powerful jetted AGN was
already in place when the Universe was <1.5 Gyr old. Such parent population
proved to be very elusive, and escaped direct detection in radio surveys so
far. High redshift blazars themselves seem to be failing in producing extended
radio-lobes, raising questions about the connection between such class and the
vaster population of radio-galaxies. We show that the interaction of the jet
electrons with the intense cosmic microwave background (CMB) radiation explains
the lack of extended radio emission in high redshift blazars and in their
parent population, helping to explain the apparently missing misaligned
counterparts of high redshift blazars. On the other hand, the emission from the
more compact and more magnetised hot spots are less affected by the enhanced
CMB energy density. By modelling the spectral energy distribution of blazar
lobes and hot spots we find that most of them should be detectable by low
frequency deep radio observations, e.g., by LOw-Frequency ARray for radio
astronomy (LOFAR) and by relatively deep X-ray observations with good angular
resolution, e.g., by the Chandra satellite. At high redshifts, the emission of
a misaligned relativistic jet, being de-beamed, is missed by current large sky
area surveys. The isotropic flux produced in the hot spots can be below ~1 mJy
and the isotropic lobe radio emission is quenched by the CMB cooling.
Consequently, even sources with very powerful jets can go undetected in current
radio surveys, and misclassified as radio-quiet AGNs.
Cosmic Ray Antiprotons from Relic Neutralinos in a Diffusion Model
Creators: name: Donato, Fiorenza
name: Nicolao Fornengo
name: Maurin, David
name: Salati, Pierre
name: Taillet, Richard
Publisher: name: INFN Open Access Repository
Year: 2003

description: We use the constraints on the diffusion parameters as obtained with stable
nuclei to calculate the cosmic antiproton flux from annihilating relic
neutralinos. We discuss the relevance of each characteristic parameter,
describing our two dimension diffusion model, on the flux of antiprotons
produced in the dark halo of our Galaxy. We estimate a two orders of magnitude
uncertainty on the flux due to the unknowledge of the propagation parameters. A
conservative and systematic evaluation of the flux in the supersymmetric
parameter space is done in order to exclude configurations providing a total
(secondary plus primary) flux in excess with observations. We also study the
effect on the flux induced by modifications in the distribution of cold dark
matter in the Galaxy.
Stable and Radioactive Nuclei in a Diffusion Model
Creators: name: Donato, Fiorenza
name: Maurin, David
name: Taillet, Richard
Publisher: name: INFN Open Access Repository
Year: 2003

description: We present the results on the source spectrum function for primary nuclei in
galactic cosmic rays, where two distinct energy dependences are used for the
source spectra. We discuss the evolution of the goodness of fit to B/C data
with the propagation parameters and also show that the results are not much
affected by a different choice for the diffusion scheme. We apply the
constraints on the diffusion scheme as derived from stable nuclei to calculate
the propagation of beta-radioactive isotopes. The diffusion model is refined to
properly take into account the effect of a local bubble in the interstellar
medium. Our calculations are compared to existing data, which prefer the local
bubble description instead of the homogeneus scheme.
title: ÐÐµÐ±-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð½ÑÐ°ÑÐ¾Ð², ÐÐ¸ÑÐ¸Ð»Ð»
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: web-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ
Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÑÑ Ð¸ÑÐµÐºÑÑÑÑ

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ web-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¿Ð¾Ð¸ÑÐºÐ° Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾Ð±ÑÑÐ¸Ð¹ (Ð²ÑÑÑÐµÑ). Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°Ð»Ð¸ÑÑ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑ Ð¸Ñ Ð´Ð¾ÑÑÐ¾Ð¸Ð½ÑÑÐ² Ð¸ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¾Ð² Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð±Ð»Ð¸ÑÐ°. ÐÑÐ»Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº web-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ° Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ.
Mid-infrared photometry of carbon stars and perspectives for surveys in
  the Magellanic Clouds from Dome-C
Creators: name: Ciprini, Stefano
name: Busso, Maurizio
Publisher: name: 2003, MemSAIt-Suppl., vol.2, p. 233
Year: 2003

description: A preliminary analysis of the data from the MSX space infrared satellite,
seems to confirm that the [8.8]-[12.5] micron color index is well correlated
with the mass-loss rates in carbon stars of our Galaxy. The extension of this
mid-infrared observation criterion to the Magellanic Clouds, with a small-size
telescope, able to perform a continuous survey from Dome-C on the Antarctic
Plateau, could be crucial to trace the local AGB population and evolution.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð±Ð°Ð·Ñ Ð¿Ð¾ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ñ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÑÐ±Ð¾ÑÐ³ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ°ÑÐµÐ²Ð°, ÐÐ½Ð½Ð°
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: Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð±Ð°Ð·Ð°
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÑÑÐ°ÑÐ¾Ð²
Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð°

description: Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð±Ð°Ð·Ñ Ð¿Ð¾ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ñ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð±Ð°Ð·Ð°, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ°Ñ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ ÑÐ°Ð¹Ð¾Ð½Ð°. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ð¹ Ð¾Ð¿ÑÑ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸. ÐÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÐ¸ Ð¶Ð¸ÑÐµÐ»ÐµÐ¹ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð² ÑÑÐµÑÐµ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð² ÑÐ°Ð¹Ð¾Ð½Ðµ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ.
Study of Plasmodiophora brassicae Wor.
Creators: name: DeWolfe, Moyra Kathleen
Publisher: name: University of British Columbia
Year: 2011

description: Reports concerning the life history of Plasmodiophora brassicae Wor. are highly conflicting. The contradictions in the literature on the subject and the difficulties encountered in the initial phase of the present investigation brought about an inquiry into the techniques employed by previous workers. Repetition of these techniques indicated that many previous experiments had not taken into consideration the problems inherent in an in vitro study of Plasmodiophora brassicae. Conclusions drawn from such experiments are thus of doubtful value. Methods described as successful by earlier investigators were employed in an attempt to stimulate germination. The germination process was not observed, and contaminants introduced with the resting spore material made it impossible to designate any one motile organism as P. brassicae. Attempts were made to obtain root hair infection. Pour methods described by previous investigators proved unsuccessful. A limited degree of infection was obtained by placing young cabbage and cauliflower seedlings in a buffered nutrient solution containing washed P. brassicae resting spores. In spite of the fact that artifacts were readily produced, early infection stages were observed and photographed and the existence of a zoosporangial stage in the root hair was confirmed. The infection rate was too low to permit intensive observations of the development of the parasite within the root hair. A proteolytic enzyme preparation was somewhat successful in increasing the infection rate. This was taken as an indication that a combination of enzymes could provide the necessary germination stimulus. Decay of the host tissues is apparently necessary to the maturation of the resting spores. Present experiments indicated that it is not feasible to separate the contaminants from these spores. As it was not possible to draw conclusions from contaminated cultures, it is concluded that the only approach of value is to provide an artificial germination stimulus to spores from clean clubs, so that the development of the parasite may take place under sterile conditions.
title: Ð Ð°Ð·Ð¼Ð¸Ð½ÐºÐ° Ð² ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¼ ÑÐ¿Ð¾ÑÑÐµ: Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¸ Ð¾ÑÐ²ÐµÑÑ
title: Warm-up in esports: questions and answers
Creators: name: ÐÐ¾ÑÑÐ¼Ð¸Ð½Ð°, ÐÐ»ÐµÐ½Ð°
name: ÐÐ°ÐºÐ°ÑÐ¾Ð², Ð®ÑÐ¸Ð¹
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ°Ð·Ð¼Ð¸Ð½ÐºÐ°
ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¹ ÑÐ¿Ð¾ÑÑ
ÐºÐ¸Ð±ÐµÑÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÐµ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ
ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¸ÑÑÐ¾Ð²ÑÐµ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ
warm-up
esports
esports disciplines
physical and digital exercises

description: Ð ÑÑÐ°ÑÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¼ ÑÐ¿Ð¾ÑÑÐ¾Ð¼ Ðº ÑÐ°Ð·Ð¼Ð¸Ð½ÐºÐµ Ð¿ÐµÑÐµÐ´ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð¸ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÑÑÑÐºÑÑÑÐ° ÑÐ°Ð·Ð¼Ð¸Ð½ÐºÐ¸ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ñ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¿Ð¾ÑÑÐ°, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÑÐ¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹. ÐÑÑÐ²Ð»ÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½Ð°Ñ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ, Ð·Ð°ÐºÐ»ÑÑÐ°ÑÑÐ°ÑÑÑ Ð² Ð¾ÑÑÑÑÑÑÐ²Ð¸Ð¸ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾ÑÑÐ¸ Ðº ÑÐ°Ð·Ð¼Ð¸Ð½ÐºÐµ Ð¿ÐµÑÐµÐ´ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð¸Ð»Ð¸ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ñ Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¼ ÑÐ¿Ð¾ÑÑÐ¾Ð¼.
description: The article presents research materials on the attitude of those involved in esports on warm-up before training and competitive activities. The structure of warm-up in various disciplines of computer sports is considered, examples of the most frequently used exercises are given. A problematic situation has been identified, consisting in the lack of knowledge and motivation to warm up before training or competitive activities among those involved in esports.
Obscured star formation at z = 0.84 with HiZELS: the relationship between star formation rate and H-alpha or ultra-violet dust extinction
Creators: name: Garn, Timothy
name: Sobral, David
name: Best, Philip N.
name: Geach, James E.
name: Smail, Ian
name: Cirasuolo, Michele
name: Dalton, Gavin B.
name: Dunlop, James S.
name: McLure, Ross J.
name: Farrah, Duncan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: [Abridged] We compare H-alpha, ultraviolet (UV) and infrared (IR) indicators of star formation rate (SFR) for a sample of z = 0.84 galaxies from the High-z Emission Line Survey (HiZELS). Using multi-wavelength diagnostics, we estimate that 5 - 11 per cent of H-alpha emitters at this redshift are active galactic nuclei. We detect 35 per cent of the H-alpha emitters individually at 24 microns, and stack the star-forming emitters on deep 24-micron images in order to calculate the typical SFRs of our galaxies. These are compared to the observed H-alpha line fluxes in order to estimate the extinction at z = 0.84, and we find a significant increase in dust extinction for galaxies with higher SFRs. We demonstrate that the local relationship between SFR and extinction is suitable for our sample, and attribute the overall increase in dust extinction for z = 0.84 galaxies to an increase in the average SFR, rather than to a change in dust properties. We calculate the UV extinction, and find a similar dependence on SFR, but no evidence for a 2175 angstrom UV bump in the dust attenuation law. We calculate the conversion between the dust attenuation of nebular and stellar radiation, gamma, and show that gamma = 0.50 +/- 0.14. The extinction / SFR relationship is shown to be applicable to galaxies with a range of morphologies and bulge-to-disk ratios, to both merging and non-merging galaxies, and to galaxies within high- and low-density environments, implying that it is a fundamental property of star-forming regions. In order to allow future studies to correct for a SFR-dependent amount of dust extinction, we present an equation to predict the extinction of a galaxy, based solely upon its observed H-alpha luminosity, and use this to recalculate the H-alpha luminosity function and star formation rate density at z = 0.84.
description: Accepted for publication in MNRAS. 15 pages, 8 figures, 4 tables
Regular Orbital Measures on Lie Algebras
Creators: name: Wright, Alex
Publisher: name: arXiv
Year: 2009
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 58C35; 22E60; 43A70

description: Let H be a regular element of an irreducible Lie Algebra g, and let mu be the orbital measure supported on the Adjoint orbit of H. We show that the k-th power of the Fourier transform of mu is in L^2(g) if and only if k > dim g/(dim g-rank g).
title: PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÐ° Ð² Ð´ÐµÐ¿ÑÑÐ°ÑÑ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð²ÑÐ±Ð¾ÑÐ¾Ð² Ð´ÐµÐ¿ÑÑÐ°ÑÐ° Ð² Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐ¾Ð¼Ð¾Ð½Ð¾ÑÐ¾Ð²)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð°, ÐÐ°Ð»ÐµÐ½ÑÐ¸Ð½Ð°
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: 2016
Subjects: Ð²ÑÐ±Ð¾ÑÑ
PR
PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ
Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½ÑÐµ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸
Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ PR
election
PR-support
political activity
election campaign
election technology
political PR

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÐ° Ð² Ð´ÐµÐ¿ÑÑÐ°ÑÑ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸. Ð ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¹, ÐµÐµ ÑÑÐ°Ð¿Ð¾Ð² Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÐ° Ð² Ð´ÐµÐ¿ÑÑÐ°ÑÑ Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð° ÐÐ½Ð´ÑÐµÑ ÐÐ²Ð°Ð½Ð¾Ð²Ð¸ÑÐ°, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ PR-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÐµ Ð² Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÐ° Ð² Ð´ÐµÐ¿ÑÑÐ°ÑÑ Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð° ÐÐ½Ð´ÑÐµÑ ÐÐ²Ð°Ð½Ð¾Ð²Ð¸ÑÐ°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð±ÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÑÐ´ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÐ° Ð² Ð´ÐµÐ¿ÑÑÐ°ÑÑ Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð° ÐÐ½Ð´ÑÐµÑ ÐÐ²Ð°Ð½Ð¾Ð²Ð¸ÑÐ° Ð² Ð²ÑÐ±Ð¾ÑÐ°Ñ Ð´ÐµÐ¿ÑÑÐ°ÑÐ° Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐ¾Ð¼Ð¾Ð½Ð¾ÑÐ¾Ð² ÑÐµÐ´ÑÐ¼Ð¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ²Ð° Ð² 2019 Ð³Ð¾Ð´Ñ.
description: This work is devoted to the PR-support political activities a candidate during the election campaign. In the theoretical part of the paper considers the concept of election campaigns, its stages and strategies. The characteristics of political activity of the candidate for deputy Andrei Ivanovich Fedorov, analyzed PR-technologies used in the election campaign of the candidate for deputy Andrei Ivanovich Fedorov. On the basis of the research we have developed a number of recommendations to improve PR-support of the candidate for deputy Andrei Ivanovich Fedorov in the elections to the municipal council of the municipality of Lomonosov seventh convocation in 2019.
Variational Bayesian Framework for Advanced Image Generation with Domain-Related Variables
Creators: name: Li, Yuxiao
name: Mazuelas, Santiago
name: Shen, Yuan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Deep generative models (DGMs) and their conditional counterparts provide a powerful ability for general-purpose generative modeling of data distributions. However, it remains challenging for existing methods to address advanced conditional generative problems without annotations, which can enable multiple applications like image-to-image translation and image editing. We present a unified Bayesian framework for such problems, which introduces an inference stage on latent variables within the learning process. In particular, we propose a variational Bayesian image translation network (VBITN) that enables multiple image translation and editing tasks. Comprehensive experiments show the effectiveness of our method on unsupervised image-to-image translation, and demonstrate the novel advanced capabilities for semantic editing and mixed domain translation.
description: 5 pages, 2 figures,
Fair Oversampling Technique using Heterogeneous Clusters
Creators: name: Sonoda, Ryosuke
Publisher: name: arXiv
Year: 2023
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Class imbalance and group (e.g., race, gender, and age) imbalance are acknowledged as two reasons in data that hinder the trade-off between fairness and utility of machine learning classifiers. Existing techniques have jointly addressed issues regarding class imbalance and group imbalance by proposing fair over-sampling techniques. Unlike the common oversampling techniques, which only address class imbalance, fair oversampling techniques significantly improve the abovementioned trade-off, as they can also address group imbalance. However, if the size of the original clusters is too small, these techniques may cause classifier overfitting. To address this problem, we herein develop a fair oversampling technique using data from heterogeneous clusters. The proposed technique generates synthetic data that have class-mix features or group-mix features to make classifiers robust to overfitting. Moreover, we develop an interpolation method that can enhance the validity of generated synthetic data by considering the original cluster distribution and data noise. Finally, we conduct experiments on five realistic datasets and three classifiers, and the experimental results demonstrate the effectiveness of the proposed technique in terms of fairness and utility.
Early phase observations of extremely luminous Type Ia Supernova 2009dc
Creators: name: Yamanaka, M.
name: Kawabata, K. S.
name: Kinugasa, K.
name: Tanaka, M.
name: Imada, A.
name: Maeda, K.
name: Nomoto, K.
name: Arai, A.
name: Chiyonobu, S.
name: Fukazawa, Y.
name: Hashimoto, O.
name: Honda, S.
name: Ikejiri, Y.
name: Itoh, R.
name: Kamata, Y.
name: Kawai, N.
name: Komatsu, T.
name: Kuroda, D.
name: Miyamoto, H.
name: Miyazaki, S.
name: Nagae, O.
name: Nakaya, H.
name: Ohsugi, T.
name: Omodaka, T.
name: Sakai, N.
name: Sasada, M.
name: Suzuki, M.
name: Taguchi, H.
name: Takahashi, H.
name: Tanaka, H.
name: Uemura, M.
name: Yamashita, T.
name: Yanagisawa, K.
name: Yoshida, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is $Δm_{15}(B)=0.65\pm 0.03$, which is one of the slowest among SNe Ia. The peak $V$-band absolute magnitude is $M_{V}=-19.90\pm 0.15$ mag even if the host extinction is $A_{V}=0$ mag. It reaches $M_{V}=-20.19\pm 0.19$ mag for the host extinction of $A_{V}=0.29$ mag as inferred from the observed Na {\sc i} D line absorption in the host. Our $JHK_{s}$-band photometry shows that the SN is one of the most luminous SNe Ia also in near-infrared wavelengths. These results indicate that SN 2009dc belongs to the most luminous class of SNe Ia, like SN 2003fg and SN 2006gz. We estimate the ejected $^{56}$Ni mass of $1.2\pm 0.3$ $\Msun$ for no host extinction case (or 1.6$\pm$ 0.4 M$_{\odot}$ for the host extinction of $A_{V}=0.29$ mag). The C {\sc ii} $λ$6580 absorption line keeps visible until a week after maximum, which diminished in SN 2006gz before its maximum brightness. The line velocity of Si {\sc ii} $λ$6355 is about 8000 km s$^{-1}$ around the maximum, being considerably slower than that of SN 2006gz, while comparable to that of SN 2003fg. The velocity of the C {\sc ii} line is almost comparable to that of the Si {\sc ii}. The presence of the carbon line suggests that thick unburned C+O layers remain after the explosion. SN 2009dc is a plausible candidate of the super-Chandrasekhar mass SNe Ia.
Cosmic Ray Energy Measurement with EAS Cherenkov Light: Experiment QUEST
  and CORSIKA Simulation
Creators: name: E. E. Korosteleva
name: L. A. Kuzmichev
name: V. V. Prosin
name: EAS-TOP COLLABORATION
Publisher: name: INFN Open Access Repository
Year: 2005

description: A new method of a primary cosmic particle energy measurement with the
extensive air shower (EAS) technique has been developed by exploiting: a) the
joint analysis of the shower size, obtained by the EAS-TOP array, and of the
EAS Cherenkov light lateral distribution (LDF), obtained by the QUEST array,
and b) simulations based on the CORSIKA code. The method is based on the strict
correlation between the size/energy ratio and the steepness of the Cherenkov
light lateral distribution and has been compared with a "classical" one based
on the Cherenkov light flux at a fixed distance (175 m) from the EAS core. The
independence of the energy measurement both on the mass of primary particle and
the hadronic interaction model used for the analysis is shown. Based on this
approach the experimental integral intensity of cosmic rays flux with energy
more than 3*10^15 eV is obtained with good systematic and statistical accuracy.
Additional file 1 of Aspartate beta-hydroxylase domain containing 1 as a prognostic marker associated with immune infiltration in skin cutaneous melanoma
Creators: name: Sun, Shiquan
name: Deng, Min
name: Wen, Juan
name: Chen, Xiaoyuan
name: Xu, Jiaqi
name: Liu, Yu
name: Wan, Huanhuan
name: Wang, Jin
name: Yan, Leping
name: He, Yong
name: Xu, Yunsheng
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Supplementary Material 1
Phason Dynamics in One-Dimensional Lattices
Creators: name: Lipp, Hansjörg
name: Engel, Michael
name: Sonntag, Steffen
name: Trebin, Hans-Rainer
Publisher: name: arXiv
Year: 2010
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In quasicrystals, the phason degree of freedom and the inherent anharmonic potentials lead to complex dynamics which cannot be described by the usual phonon modes of motion. We have constructed simple one-dimensional model systems, the dynamic Fibonacci chain (DFC) and approximants thereof. They allow us to study the dynamics of periodic and quasiperiodic structures with anharmonic double well interactions both by analytical calculations and by molecular dynamics simulations. We found soliton modes like breathers and kink solitons and we were able to obtain closed analytical solutions for special cases, which are in good agreement with our simulations. Calculation of the specific heat shows an increase above the Dulong-Petit value, which is due to the anharmonicity of the potential and not caused by the phason degree of freedom.
description: 13 pages, 18 figures
title: Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. Ð§. 1
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº ÑÑÑÐ´Ð¾Ð² Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸
titleType: Subtitle
Creators: name: "Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: Ð½Ð°ÑÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐ±Ð»Ð¸ÐºÑÑÑÑÑ ÑÑÐ°ÑÑÐ¸ Ð¿Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ð¼ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð², Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°ÑÐµÐ´Ð°Ð½Ð¸ÑÑ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸Â». Ð¡ÑÐ°ÑÑÐ¸ Ð¾ÑÑÐ°Ð¶Ð°ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸, Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸, ÑÐµÑÑÑÑÐºÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ
ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½Ð° Ð¼Ð¸ÐºÑÐ¾- Ð¸ Ð¼Ð°ÐºÑÐ¾ÑÑÐ¾Ð²Ð½ÑÑ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ¾Ð¼.
Multi-Granularity Detector for Vulnerability Fixes
Creators: name: Nguyen, Truong Giang
name: Le-Cong, Thanh
name: Kang, Hong Jin
name: Widyasari, Ratnadira
name: Yang, Chengran
name: Zhao, Zhipeng
name: Xu, Bowen
name: Zhou, Jiayuan
name: Xia, Xin
name: Hassan, Ahmed E.
name: Le, Xuan-Bach D.
name: Lo, David
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cryptography and Security (cs.CR)
subject: Artificial Intelligence (cs.AI)
subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: With the increasing reliance on Open Source Software, users are exposed to third-party library vulnerabilities. Software Composition Analysis (SCA) tools have been created to alert users of such vulnerabilities. SCA requires the identification of vulnerability-fixing commits. Prior works have proposed methods that can automatically identify such vulnerability-fixing commits. However, identifying such commits is highly challenging, as only a very small minority of commits are vulnerability fixing. Moreover, code changes can be noisy and difficult to analyze. We observe that noise can occur at different levels of detail, making it challenging to detect vulnerability fixes accurately. To address these challenges and boost the effectiveness of prior works, we propose MiDas (Multi-Granularity Detector for Vulnerability Fixes). Unique from prior works, Midas constructs different neural networks for each level of code change granularity, corresponding to commit-level, file-level, hunk-level, and line-level, following their natural organization. It then utilizes an ensemble model that combines all base models to generate the final prediction. This design allows MiDas to better handle the noisy and highly imbalanced nature of vulnerability-fixing commit data. Additionally, to reduce the human effort required to inspect code changes, we have designed an effort-aware adjustment for Midas's outputs based on commit length. The evaluation results demonstrate that MiDas outperforms the current state-of-the-art baseline in terms of AUC by 4.9% and 13.7% on Java and Python-based datasets, respectively. Furthermore, in terms of two effort-aware metrics, EffortCost@L and Popt@L, MiDas also outperforms the state-of-the-art baseline, achieving improvements of up to 28.2% and 15.9% on Java, and 60% and 51.4% on Python, respectively.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
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¡ÑÐ°ÑÐ¾ÑÐµÐ»ÑÑÐºÐ¸Ð¹, Ð Ð¾Ð¼Ð°Ð½
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: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾ - Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
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description: ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
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Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
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title: Ð¡Ð²ÐµÑÑ Ð²ÑÑÐ¾ÐºÐ¸Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ "Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°"
titleType: Subtitle
Creators: name: ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ¾Ð², ÐÐµÐ¾ÑÐ³Ð¸Ð¹
name: ÐÐ¾ÑÐ°ÑÐ¾Ð², Ð®ÑÐ¸Ð¹
name: ÐÐ°ÑÐºÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¢Ð¸ÑÐºÐ¾Ð², ÐÐ°ÑÐ¸Ð»Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð»Ð¸Ð½Ð¸Ð¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÐµ
ÐÑÑÐ¾ÐºÐ¸Ðµ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ (ÑÐ»ÐµÐºÑÑ.)

description: ÐÑÑÑ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð²Ð¾Ð·Ð´ÑÑÐ½ÑÑ Ð¸ ÐºÐ°Ð±ÐµÐ»ÑÐ½ÑÑ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÐµÑÐµÐ´Ð°Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð¸ ÑÐ²ÐµÑÑÐ²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹, Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ Ð»Ð¸Ð½Ð¸Ð¹ ÑÐ°ÐºÐ¾Ð³Ð¾ ÐºÐ»Ð°ÑÑÐ° Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â». ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð² ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ñ.
title: Ð¢ÐµÐ¾ÑÐ¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¾Ð´, ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐÐ
Year: 1983
Subjects: ÐÐ¸ÑÐµÐ¹Ð½Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑ "Ð¢ÐµÐ¾ÑÐ¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²" Ð¸ "ÐÐ¸ÑÐµÐ¹Ð½Ð¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾". ÐÐ·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¾Ð±ÑÐ¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐµ Ð¿ÑÐ¾ÑÐµÐºÐ°Ð½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð»Ð¸ÑÐµÐ¹Â­Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÑÐ¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº, Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÐµ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÐµ (Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð­ÐÐ) Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ°, ÑÐµÑÐ½Ð¸ÐºÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð°Ñ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑÑÐ°, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¾Ð¿ÑÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¾ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐ¼ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ¾Ð¼ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð².
A Prelimanary Exploration on component based software engineering
Creators: name: Basha, N Md Jubair
name: Ganapathy, Gopinath
name: Moulana, Mohammed
Publisher: name: arXiv
Year: 2023
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Component-based software development (CBD) is a methodology that has been embraced by the software industry to accelerate development, save costs and timelines, minimize testing requirements, and boost quality and output. Compared to the conventional software development approach, this led to the system's development being completed more quickly. By choosing components, identifying systems, and evaluating those systems, CBSE contributes significantly to the software development process. The objective of CBSE is to codify and standardize all disciplines that support CBD-related operations. Analysis of the comparison between component-based and scripting technologies reveals that, in terms of qualitative performance, component-based technologies scale more effectively. Further study and application of CBSE are directly related to the CBD approach's success. This paper explores the introductory concepts and comparative analysis related to component-based software engineering which have been around for a while, but proper adaption of CBSE are still lacking issues are also focused.
title: ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ°ÑÑÑÑÐ° ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÑÐµÐ¼ÑÑ Ð½Ð°Ð±ÐµÑÐµÐ¶Ð½ÑÑ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¸Ð¶ÐµÐ³Ð¾ÑÐ¾Ð´ÑÐºÐ¾Ð³Ð¾ ÑÐµÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ°)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¡Ð¾ÑÐ¾ÐºÐ¾Ð»ÐµÑÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
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Ð¾ÑÑÑ ÑÐµÑÐ½ÑÐµ
ÐÐ°Ð±ÐµÑÐµÐ¶Ð½ÑÐµ

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÐµÐ´Ð¸Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº ÑÐ°ÑÑÐµÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð½Ð°Ð±ÐµÑÐµÐ¶Ð½ÑÑ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ: Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ ÑÐ¸Ð¿ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ (Ð·Ð°Ð´Ð°Ð½Ð¸Ðµ) Ð¸ Ð´Ð°Ð½Ð¾ ÐµÐ³Ð¾ ÐºÑÐ°ÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ; ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð° Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð³Ð°Ð±Ð°ÑÐ¸ÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ, Ð²ÐºÐ»ÑÑÐ°Ñ Ð³Ð»ÑÐ±Ð¸Ð½Ñ Ð¿Ð¾Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð´Ð±Ð¾Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð²; Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð²Ð½ÐµÑÐ½Ð¸Ðµ Ð³Ð¾ÑÐ¸Ð·Ð¾Ð½ÑÐ°Ð»ÑÐ½ÑÐµ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ (Ð¾Ñ Ð³ÑÑÐ½ÑÐ°, ÑÐ²Ð°ÑÑÐ¾Ð²Ð½ÑÐµ, ÐºÑÐ°Ð½Ð¾Ð²ÑÐµ) Ð¸ Ð²ÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½ÑÐµ (Ð¾Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð²ÐµÑÐ°, ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ°Ð²Ð½Ð¾Ð¼ÐµÑÐ½Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐµ, ÐºÑÐ°Ð½Ð¾Ð²ÑÐµ) Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ Ð½Ð° ÑÐ°ÑÑÐµÑÐ½ÑÐ¹ ÑÑÐ°ÑÑÐ¾Ðº Ð´Ð»Ð¸Ð½Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ; Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÑÑ ÐºÐ¾ÑÑÐµÐºÑÐ¸ÑÐ¾Ð²ÐºÐ° Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ Ð³ÑÑÐ½ÑÐ° Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ Ð´ÐµÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ ÑÑÐµÐ½ÐºÐ¸ Ð¸Ð»Ð¸ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ ÐµÐµ Ð½Ð¸Ð¶Ð½ÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÐ° Ð¸ Ñ.Ð´.; Ð²ÑÑÐ¸ÑÐ»ÑÑÑÑÑ Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ SCAD ÑÑÐ¸Ð»Ð¸Ñ (M, Q, N, R) Ð¸ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ (f) ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¾Ñ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð²ÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½ÑÑ Ð¸ Ð³Ð¾ÑÐ¸Ð·Ð¾Ð½ÑÐ°Ð»ÑÐ½ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº; Ð´ÐµÐ»Ð°ÐµÑÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°Ð±Ð»Ð¸ÑÐ°.
Interface reactions between iron alloys and magnesium oxide single crystals
Creators: name: Rose, Daneil Joseph
Publisher: name: University of British Columbia
Year: 2011

description: The wettability of Mg0 by liquid iron was studied using the sessile drop technique in vacuo at 1550°C. Specimens of vacuum-cast iron were melted on single crystals of optical-grade magnesium oxide. Tests were limited to two minutes because of iron volatilization. Chemical reaction at the liquid-vapor interface caused the contact angle to decrease from 117° to 65° during the first minute. Reaction between the iron and oxygen provided through the dissociation of Mg0 resulted in formation of an Fe0 layer over the drop surface. The Fe0 was drawn to the base of the drop where it accumulated as an annular Interfacial deposit. After solidification, the Fe0 decomposed to magnetite with separation of iron. Within the peripheral annulus the interface showed no sign of chemical attack. This effect was related to formation of a protective interfacial monolayer from electropositive impurities initially present in the iron. The major constituent of the monolayer appeared to be silicon although positive identification was not achieved. Chemical reaction occurred in each case where alloying additions to the iron of Ti, V, Cr, Nb, Ta, and Zr were made. Variation of contact angle with concentration was studied. Both V and Cr improved the wettability. The effect of Zr, Ti, Nb, and Ta on the wettability was not determined because oxide deposits around the basal periphery of the drops restricted expansion. Complete interfacial attack was observed with additions of Zr, Ti, and V whereas additions of Nb, Ta, and Cr resulted in an annular interfacial deposit around the drop perimeter similar to the pure Fe-Mg0 specimens. This phenomena supported the existence of an interfacial monolayer.