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  • ASTRONOMY  (5)
  • growth  (1)
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  • 1
    ISSN: 1573-5117
    Keywords: grapsid crabs ; detritivory ; growth ; survival ; assimilation efficiency
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract The growth performance of adult individuals of the detritivorous mangrove grapsid crabs Chiromanthes bidens and Parasesarma plicata common in the Mai Po marshes, Hong Kong, was followed in a long-term laboratory rearing experiment (10 months). Individual crabs' moulting frequency, growth increment and mortality when fed four kinds of leaf litter available in their natural habitats, viz. brown (two weeks of decomposition) and yellow (fresh litter) Kandelia candel, and brown and yellow Avicennia marina were followed. The survival period was strongly related to litter type when the data from both crab species were pooled, being longest for crabs fed with brown Avicennia marina, followed by brown Kandelia candel 〉 yellow Avicennia marina 〉 yellow Kandelia candel. A higher proportion of crabs moulted twice when yellow Avicennia marina was supplied, but more crabs moulted for a third time when fed with brown Avicennia marina. The growth increment of the two species of crabs after moulting was found to be significantly related to their pre-moult size (ANOVA, P〈0.05), but effects of the four treatments were non-significant. Increment of Chiromanthes bidens was significantly greater than that of Parasesarma plicata under the brown Kandelia candel treatment. Litter treatment has no effect on the time taken for the crabs to moult, only in the case of the yellow Avicennia marina treatment did Parasesarma plicata take a longer time to moult a second time.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2013-08-31
    Description: The Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory (GRO) is sensitive in the energy range from about 20 MeV to about 30,000 MeV. Electron-positron pair production by incident gamma photons is utilized as the detection mechanism. The pair production occurs in tantalum foils interleaved with the layers of a digital spark chamber system; the spark chamber records the tracks of the electron and positron, allowing the reconstruction of the arrival direction of the gamma ray. If there is no signal from the charged particle anticoincidence detector which surrounds the upper part of the detector, the spark chamber array is triggered by two hodoscopes of plastic scintillators. A time of flight requirement is included to reject events moving backward through the telescope. The energy of the gamma ray is primarily determined by absorption of the energies of the electron and positron in a 20 cm deep NaI(Tl) scintillator.
    Keywords: ASTRONOMY
    Type: The Compton Observatory Science Workshop; p 116-125
    Format: application/pdf
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  • 3
    Publication Date: 2019-06-28
    Description: The quasar 3C 273 was detected by the Compton Observatory Satellite (COS-B) in the 1970's. Energetic Gamma Ray Experiment Telescope (EGRET) observations of this sky region in Jun. and Oct. 1991 revealed a flux from 3C 273 lower than that measured by COS-B. The flux observed by EGRET in the June period is approximately 0.0000003/sq cm(exp -2) sec(exp -1) for energies greater than 100 MeV. During the Oct. observation it appears to be even lower. For the first observation a preliminary spectrum was derived which was a photon index of 2.4.
    Keywords: ASTRONOMY
    Type: Max-Planck-Inst. fuer Physik und Astrophysik, EGRET Mission and Data Analysis; 3 p
    Format: application/pdf
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  • 4
    Publication Date: 2019-07-13
    Description: The Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory (CGRO) covers the high energy gamma ray energy range, approximately 30 MeV to 30 GeV, with a sensitivity considerably greater than earlier high energy gamma-ray satellites. Thus far, 4 pulsars have been detected and their properties measured, including in 3 cases the energy spectrum as a function of phase. The details of the galactic plane are being mapped and a spectra of the center region has been obtained in good agreement with that expected from cosmic ray interactions. The Magellanic clouds have been examined with the Large Magellanic Cloud (LMC) having been detected at a level consistent with it having a cosmic ray density compatible with quasi-stable equilibrium. Sixteen Active Galactic Nuclei (AGN's) have been seen thus far with a high degree of certainty including 12 quasars and 4 BL Lac objects, but no Seyferts. Time variation has been detected in some of these AGN's
    Keywords: ASTRONOMY
    Type: Advances in Space Research (ISSN 0273-1177); 13; 12; p. (12)637-(12)646
    Format: text
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  • 5
    Publication Date: 2019-07-13
    Description: The Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory (CGRO) observed high-energy gamma rays from PKS 0537-441 during observations in 1991 July-August. Upper limits from later EGRET observations suggest time variability.
    Keywords: ASTRONOMY
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 410; 1; p. 87-89.
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  • 6
    Publication Date: 2019-07-13
    Description: The quasar 3C 273 was detected by COS-B in the 1970's. EGRET observations of this sky region in June and October 1991 revealed a flux from 3C 273 lower than that measured by COS-B. The flux observed by EGRET in the June period is approximately 3 x 10 exp -7/sq cm s for energies greater than 100 MeV. During the October observation it appears to be even lower. For the first observation a preliminary spectrum which has a photon index of 2.4 has been derived.
    Keywords: ASTRONOMY
    Type: Astronomy and Astrophysics Supplement Series (ISSN 0365-0138); 97; 1; p. 101-103.
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