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Pires, S.; Starck, J.L.; Refregier, A.; Mathur, S.
CEA Saclay, Dept. d'Astrophysique, de Physique des Particules, de Physique Nucleaire et de l'Instrumentation Associee, 91- Gif sur Yvette (France)2004
CEA Saclay, Dept. d'Astrophysique, de Physique des Particules, de Physique Nucleaire et de l'Instrumentation Associee, 91- Gif sur Yvette (France)2004
AbstractAbstract
[en] Weak gravitational lensing provides a unique method to map directly the distribution of dark matter in the universe. Several methods are generally used to derive the lensing shear from the shapes of background galaxies, but the shear map obtained is always noisy. In this report we have tested different methods of de-noising: the Gaussian filter, the Wiener filter and the multi-scale entropy method (MEM). We notice that the Wiener filter with an additional soft threshold is the one that gives the filtered mass map nearest to the real mass map according to the standard deviation estimator. The Gaussian filter is the one that gives the coarsest result: the main peaks are found but the edges remain vague. The Wiener filter gives good results in the Fourier space but is better when applied in the wavelet space. We can say that the MEM is the best method we have tested as it enables us to detect all the main structures of the mass map without doing too many false detections. (A.C.)
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Jul 2004; 36 p; 8 refs.
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[en] We present the results of two observations of the bright Seyfert 1 galaxy NGC 3516, obtained with BeppoSAX in 1996 November and 1997 March. Useful signal is detected between 0.2 and 60 keV, allowing for the first time the simultaneous observation of all main spectral features. The source was brighter by a factor 2 at the second epoch of observation. Both spectra present a strong Fe Kα line, and a reflection hump at high energy. An absorption edge at 0.8 keV is visible in the later spectrum, but not in the earlier one, indicating that this feature is strongly variable
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Workshop on the active X-ray sky: Results from BeppoSAX and RXTE; Rome (Italy); 21-24 Oct 1997; S0920563298002710; Copyright (c) 1999 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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[en] The United States Department of Energy (DOE) conducts through its operating contractors major nuclear research, development, and production operations at nearly 30 installations. Emission and environmental monitoring programmes conducted at these sites are intended to ensure effective effluent controls and compliance with applicable radiation standards. Radionuclide emissions from DOE facilities are reported annually to a central computer-based effluent information system. This system enables DOE management to identify emission sources and observe trends in emission levels. Emissions to the environment from all DOE installations in 1981 totalled 1.9 million curies, predominantly short-lived activity, noble gases, and tritium. Significant trends in emissions and population exposures resulting from the emissions are discussed. Each DOE installation prepares an annual environmental monitoring report summarizing radionuclide emissions and computed radiation dose to the public within an 80 km radius. Actual measurements of radioactivity in human exposure pathways are used whenever possible to calculate dose to the public. Often it is necessary to calculate doses using effluent and meteorological data and appropriate dispersion equations. Calculations include the maximum individual dose and the 80 km population dose. Assessments of population dose at DOE installations in 1981 indicate that offsite exposure of the maximum individual did not exceed 10% of the 500 mrem limit at any site, and generally was less than 1% at most sites. For 1981, the calculated population whole-body dose within an 80 km radius of individual DOE sites ranged up to 120 man.rem and totalled about 230 man.rem. Calculated population doses from DOE operations are discussed, including radionuclide-specific contributions to public doses and year to year trends. A brief review is included of the DOE reporting systems for effluent releases and environmental doses. (author)
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International Atomic Energy Agency, Vienna (Austria); Proceedings series; 466 p; ISBN 92-0-020684-0; ; 1984; v. 5 p. 127-141; IAEA; Vienna (Austria); International conference on radioactive waste management; Seattle, WA (USA); 16-20 May 1983; IAEA-CN--43/299; CONTRACT DE-AC06-76RLO 1830
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AbstractAbstract
No abstract available
Original Title
Sostav i konstanty ustojchivosti kompleksov niobiya s ferronom
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For English translation see the journal Russ. J. Inorg. Chem.
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Zhurnal Neorganicheskoj Khimii; v. 19(8); p. 2288-2291
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AZINES, CARBOXYLIC ACID SALTS, COMPLEXES, DISPERSIONS, HETEROCYCLIC COMPOUNDS, HYDROXY COMPOUNDS, MIXTURES, ORGANIC ACIDS, ORGANIC COMPOUNDS, ORGANIC HALOGEN COMPOUNDS, ORGANIC IODINE COMPOUNDS, ORGANIC NITROGEN COMPOUNDS, ORGANIC SULFUR COMPOUNDS, PYRIDINES, QUINOLINES, REAGENTS, SOLUTIONS, SULFONIC ACIDS, SYNTHESIS, TRANSITION ELEMENT COMPLEXES, TRANSITION ELEMENT COMPOUNDS
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[en] Female Swiss albino mice were exposed at 1, 3 or 6 weeks of age respectively to sublethal doses (0.6, 1.2 and 2.4 Gy) of gamma radiation in the presence or absence of 2-mercaptopropionylglycine (MPG). Ovaries were histologically examined at different intervals after irradiation and the follicles were counted. Most follicular depletion had occurred already at postirradiation day 1 and the depletion then gradually continued. At day 35 after irradiation a few follicles could still be found in mice exposed at 1 week of age while all follicles were eliminated in mice exposed at 3 and 6 weeks of age. In MPG-treated animals the depletion of follicles was significantly less pronounced and obviously MPG to some degree protected the ovaries from radiation damage. (orig.)
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AMINO ACIDS, ANIMALS, BIOLOGICAL EFFECTS, BODY, CARBOXYLIC ACIDS, DRUGS, ELECTROMAGNETIC RADIATION, FEMALE GENITALS, GONADS, IONIZING RADIATIONS, IRRADIATION, MAMMALS, ORGANIC ACIDS, ORGANIC COMPOUNDS, ORGANIC SULFUR COMPOUNDS, ORGANS, RADIATION EFFECTS, RADIATIONS, RESPONSE MODIFYING FACTORS, RODENTS, VERTEBRATES
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No abstract available
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Published in summary form only, 6 refs.
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Indian Journal of Chemistry; v. 11(12); p. 1327-1328
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[en] We present a statistical analysis of the Chandra observation of the source field around the 3C 295 galaxy cluster (z=0.46). The logN-logS of this field is in good agreement with that computed for the Chandra Deep Field South in this work and in previous ones. Nevertheless, the logN-logS computed separately for the four ACIS-I chips reveals that there is a significant excess of sources to the North-North East and a void to the South of the central cluster. Such an asymmetric distribution is confirmed by the two-dimensional Kolmogorov-Smirnov test, which excludes (P∼3%) a uniform distribution. In addition, a strong spatial correlation emerges from the study of the angular correlation function of the field: the angular correlation function is above that expected for X-ray sources on a few arcmin scales. In synthesis, the present analysis may indicate a filament of the large scale structure of the Universe toward 3C 295. This kind of study may open-up a new way to map (with high efficiency) high-density peaks of large scale structures at high redshift
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2. BeppoSAX conference on the restless high-energy universe; Amsterdam (Netherlands); 5-9 May 2003; S0920563204000635; Copyright (c) 2004 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
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AbstractAbstract
[en] Interactions of 5 GeV p-bar with light nuclei in emulsion have been investigated here. The features studied are multiplicity, pseudo-rapidity and azimuthal angle distributions of the secondary particles. The results have been compared with p-nucleus interactions
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[en] The preparation and properties of dysprosium and holmium derivatives of mono-, di- and tri-ethanolamine derivatives are described. Compounds of general formulae: Ln(OPrsup(i))2(mea), Ln(OPrsup(i))(mea)2, Ln(mea)3, Ln(OPrsup(i))(dea), Ln2(dea)3, Ln(dea)(deaH) and Ln(tea) (where Ln = Dy or Ho and mea, dea and tea are the anions of respective ethanolamine) were obtained and characterized by elemental analysis and IR spectra. (author)
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Journal of Inorganic and Nuclear Chemistry; ISSN 0022-1902; ; v. 43(9); p. 2152-2154
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[en] Six week old male Swiss albino mice taken from an inbred colony were irradiated with 0.6 and 1.2 Gy of low 60Co gamma rays in the presence and absence of MPG. Results indicated the infliction of radiation insult and subsequent repair in the testes to be dose dependent, that is higher the dose greater the damage and sluggish the reparative activity. A greater number of suviving germ cells in the experimental tests with fewer dead cells reflected the protective efficiency of the drug against radiation damage to the cell population. Thus MPG not only protects against radiation-induced cell death and depletion but also chances the mitotic rate of the stem cells by which an accelerated recovery was brought about. (author)
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AMINO ACIDS, ANIMALS, BETA DECAY RADIOISOTOPES, BETA-MINUS DECAY RADIOISOTOPES, BIOLOGICAL EFFECTS, BODY, CARBOXYLIC ACIDS, CELL DIVISION, COBALT ISOTOPES, DRUGS, ELECTROMAGNETIC RADIATION, EXTERNAL IRRADIATION, GONADS, INTERMEDIATE MASS NUCLEI, IONIZING RADIATIONS, IRRADIATION, ISOMERIC TRANSITION ISOTOPES, ISOTOPES, MALE GENITALS, MAMMALS, MINUTES LIVING RADIOISOTOPES, NUCLEI, ODD-ODD NUCLEI, ORGANIC ACIDS, ORGANIC COMPOUNDS, ORGANIC SULFUR COMPOUNDS, ORGANS, RADIATION EFFECTS, RADIATIONS, RADIOISOTOPES, RADIOPROTECTIVE SUBSTANCES, RESPONSE MODIFYING FACTORS, RODENTS, THIOLS, VERTEBRATES, YEARS LIVING RADIOISOTOPES
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