May 1973
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.243...25c&link_type=abstract
Nature, Volume 243, Issue 5401, pp. 25-26 (1973).
Physics
3
Scientific paper
Carswell and Strittmatter, reporting the high redshift1 they measured for OH471, do not quote the accurate radio and optical coordinates which were the basis of its identification. These coordinates are: Radio α(1950) = 06 h 42 min 53.3 s +/-0.2s δ(1950)=44° 54' 33'' +/- 1'' Optical α(1950)=06 h 42 min 53.1 s +/-0.1 s δ(1950) =44° 54' 31'' +/-1'' The radio position was measured by the method described by Adgie et al.2 except that an interferometer spacing of only 1,300 wavelengths was used. The optical position was measured on the prints of the Palomar Sky Survey relative to AGK2 stars: the accuracy achieved was estimated from the distribution of radio-optical position differences obtained in a large number of similar measurements.
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