M. Rozas , A. Zurita , J. E. Beckman, PASA, 15 (1), 159
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file.
| Next Section: Data analysis Title/Abstract Page: QUANTIFYING THE IONIZING FLUX Previous Section: QUANTIFYING THE IONIZING FLUX | Contents Page: Volume 15, Number 1 |
Observations
All the galaxies were observed through the TAURUS camera on the 4.2m William Herschel Telescope, La Palma. Calibrated photometric sub-arcsec images in appropriately red-shifted H
were obtained by subtracting a nearby continuum image from that through the H filter. Absolute fluxes were determined via distances derived using H
= 75 km s
Mpc.
| Next Section: Data analysis Title/Abstract Page: QUANTIFYING THE IONIZING FLUX Previous Section: QUANTIFYING THE IONIZING FLUX | Contents Page: Volume 15, Number 1 |
© Copyright Astronomical Society of Australia 1997 ASKAP
Public