The H
- P. A. James
- N. S. Shane
- J. E. Beckman
- A. Cardwell
- C. A. Collins
- J. Etherton
- R. S. de Jong
- K. Fathi
- J. H. Knapen
- R. F. Peletier
- S. M. Percival
- D. L. Pollacco
- M. S. Seigar
- S. Stedman
- I. A. Steele
DOIAbstract
We discuss the selection and observations of a large sample of nearby galaxies, which we are using to quantify the star formation activity in the local Universe. The sample consists of 334 galaxies across all Hubble types from S0/a to Im and with recession velocities of between 0 and 3000 km s-1. The basic data for each galaxy are narrow band H$\alpha +$[Ni
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