SN1994I at 15.2 GHz
G.G. Pooley and D.A. Green
The figure and data below give the radio flux density of SN1994I at 15.2 GHz,
as observed by the Ryle Telescope.
- The data below are for Stokes parameter I+Q, and have been
calibrated based on a flux density of 1.70 Jy for 3C48.
- The date is given for the centre of each observation, which vary in
duration, but are typically 1 to 2 hours long. The uncertainty in flux
densities do not include uncertainties in the flux density calibration.
The data are available as an ascii file. If you
wish to use these data, please cite as a private communication from Pooley G.G.
& Green D.A. for these data.
