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  • 1
    ISSN: 1433-2965
    Keywords: DXA ; Postmenopausal women ; Premenopausal women ; Radiographic absorptiometry of the phalanges ; SXA
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Notes: Abstract We present baseline bone densitometry from the Early Postmenopausal Interventional Cohort study (EPIC, sponsored by Merck, Sharp & Dohme) for the first time, in which 1609 women from England, Oregon, Hawaii and Denmark are participating to investigate the efficacy of daily oral alendronate to prevent early postmenopausal bone loss. We compared radiographic absorptiometry (RA) of the phalanges for bone mineral density (BMD) measurement with single-energy X-ray absorptiometry (SXA) of the distal forearm, and dual-energy X-ray absorptiometry (DXA) of the lumbar spine, proximal femur and distal forearm. In a random subgroup of 308 women, aged 45–60 years, on average 6 years since menopause (YSM), bone densitometry was measured once at baseline by RA of the phalanges besides the mandatory measurements by DXA. Bone densitometry was furthermore measured by SXA at the Danish site (89 women). Sixty-eight of the women had duplicate measurements performed within 1–3 weeks to evaluate the short-term precision error (CV%). One hundred and one healthy premenopausal women, aged 25–48 years, were recruited at the Danish and Hawaiian sites to establish a reference group. The precision error was 1.5% for RA of the phalanges and in the range 1.0–2.2% for SXA and DXA. BMD by RA correlated with BMD measured by SXA and DXA in the range 0.45〈r〈0.72 (p〈0.001). In conclusion, bone densitometry by RA of the phalanges is highly correlated with bone densitometry by SXA and DXA. RA of the phalanges has a short-term precision error comparable to that of SXA and DXA.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1572-946X
    Keywords: GRB radio counterparts ; BACODINE
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The Cambridge Low Frequency Synthesis Telescope (CLFST) is being used to search for prompt radio emission from GRBs at 151 MHz. For this search a special observing mode has recently been developed; the antennas of the CLFST are split into seven groups which are spaced about 30° apart. When triggered by the real-time signals from the BACODINE system the antennas are slewed to the GRB position, with data being sampled at 1.5 or 3-s intervals. The antennas slew at about 10° per minute, so that an appreciable fraction of the sky can be accessed on timescales of a few minutes - any prompt radio emission from a GRB might be delayed by this timescale due to propagation effects.
    Type of Medium: Electronic Resource
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