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  • 1
    ISSN: 1432-0649
    Keywords: 33.00 ; 42.65 ; 42.80
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We report direct measurements of the excited singlet state absorption cross section and the associated nonlinear refractive cross section using picosecond pulses at 532 nm in solutions of phthalocyanine and naphthalocyanine dyes. By monitoring the transmittance and far field spatial beam distortion for different pulsewidths in the picosecond regime, we determine that both the nonlinear absorption and refraction are fluence (energy per unit area) rather than irradiance dependent. Thus, excited state absorption (ESA) is the dominant nonlinear absorption process, and the observed nonlinear refraction is also due to real population excitation.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    European journal of clinical pharmacology 51 (1996), S. 123-126 
    ISSN: 1432-1041
    Keywords: Key words Angiotensin converting enzyme inhibitors ; Angiooedema ; Urticaria
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Medicine
    Notes: Abstract Objective: To review reports of angiooedema and urticaria associated with angiotensin converting enzyme inhibitors (ACEI) in the New Zealand Centre for Adverse Reactions Monitoring and Intensive Medicines Monitoring Programme (IMMP) database. Methods: Adverse reaction reports describing angiooedema and/or urticaria between April 1981 and December 1994 were examined. Captopril, enalapril and lisinopril were intensively monitored on the IMMP during this period. Results: Of a total of 116 reports there were 68 reports of angiooedema and 37 of urticaria alone and 11 where angiooedema and urticaria occurred in the same patient. The total number of patients is unknown, but cohorts of patients on captopril, enalapril and lisinopril in the IMMP were 16342, 25686 and 11235, totalling 53263 patients. There were 63 reports of angiooedema/urticaria in patients monitored on the IMMP, giving a reported rate of 1.2/1000 (0.9–1.5). Forty seven reactions occurred between 3 weeks and 4 years after commencement of therapy. Severe angiooedema occurred in 9 patients with early-onset angiooedema and 6 with late-onset angiooedema. There were no deaths. Seventeen patients had up to 12 episodes before diagnosis. Angiooedema/ urticaria occurred without gender preference. Although a dose relationship was not apparent, 3 patients developed angiooedema or urticaria after an increase in dose. Conclusion: Although reactions are more common shortly after initiation of ACEI therapy, late onset reactions may be less well recognised. Clinicians should be reminded, and ACEI data sheets should emphasise, that onset may be delayed for weeks or months, that patients may have multiple episodes with long symptom free intervals, and that angiooedema may occur with or without urticaria.
    Type of Medium: Electronic Resource
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  • 3
    Publication Date: 2019-07-13
    Description: The stellar initial mass function (IMF), which is often assumed to be universal across unresolved stellar populations, has recently been suggested to be bottom-heavy for massive ellipticals. In these galaxies, the prevalence of gravity-sensitive absorption lines (e.g., Na I and Ca II) in their near-IR spectra implies an excess of low-mass (m 〈 or approx. = 0.5 Stellar Mass) stars over that expected from a canonical IMF observed in low-mass ellipticals. A direct extrapolation of such a bottom-heavy IMF to high stellar masses (m 〉 or approx. = 8 Stellar Mass) would lead to a corresponding deficit of neutron stars and black holes, and therefore of low-mass X-ray binaries (LMXBs), per unit near-IR luminosity in these galaxies. Peacock et al. searched for evidence of this trend and found that the observed number of LMXBs per unit K-band luminosity (N/LK) was nearly constant. We extend this work using new and archival Chandra X-ray Observatory and Hubble Space Telescope observations of seven low-mass ellipticals where N/LK is expected to be the largest and compare these data with a variety of IMF models to test which are consistent with the observed N/LK. We reproduce the result of Peacock et al., strengthening the constraint that the slope of the IMF at m 〉 or approx. = 8 Stellar Mass must be consistent with a Kroupa-like IMF. We construct an IMF model that is a linear combination of a Milky Way-like IMF and a broken power-law IMF, with a steep slope (alpha1 = 3.84) for stars 〈 0.5 Stellar Mass (as suggested by near-IR indices), and that flattens out (alpha2 = 2.14) for stars 〉 0.5 Stellar Mass, and discuss its wider ramifications and limitations.
    Keywords: Astrophysics
    Type: GSFC-E-DAA-TN45844 , The Astrophysical Journal (ISSN 2041-8205) (e-ISSN 2041-8213); 835; 2; 183
    Format: text
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