Program description

We divide the description of WHISP into four parts. The motivation to start this program is described in the Overview and is also reviewed in the Program report 1993. The main part of WHISP consists of the 21cm HI-line observations of nearby galaxies. The way the galaxies are being selected for observing is given in the Definition of the galaxy sample. How the galaxies are observed at the WSRT is described in Observing parameters.


Program report 1993

Definition of the galaxy sample

Observing parameters