Surveying the Universe
On the normalization of PRFs
Yesterday I said that the PRF for a map in Jy/beam (or similar) should be normalized so that that peak is 1. But this is true only for an idealised (not pixelated) PRF, or if the map has infinitesimally small pixels.
If the pixels are larger than infinitesimal, as is generally the case, then the maximum value of the pixelated PRF will be the average value over the pixel, which will be less than 1.
For example, if the PRF is a two-dimensional Gaussian, centred on
, with standard deviation
, then the value in a pixel with
and
will be



Ugh. Let's make that simpler. For a PRF centred on
, and a pixel
, this is

As an example, the fairly-Gaussian beam for the Herschel Space Observatory SPIRE instrument has an FWHM of around 18", which corresponds to a standard deviation of around
. If we make a Jy/beam map with pixel size 6", then the peak value for a 1 Jy point source in the centre of a pixel will be

No big deal really...
| Print article | This entry was posted by Anthony on 4 Sep 2009 at 11.59 am, and is filed under Research. Follow any responses to this post through RSS 2.0. You can leave a response or trackback from your own site. |

I live in York and I