Imaging Survey Michelle Buxton, Michael Bessell and Bob Watson, PASA, 15 (1), 24
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: Acknowledgements Title/Abstract Page: The MSSSO Wide Field Previous Section: Comparison with MOST Galactic | Contents Page: Volume 15, Number 1 |
Conclusion
The Wide Field H
Survey in conjunction with the MOST radio survey will provide valuable information to the astronomical community on the nature of excitation in many of the continuum sources in the Galaxy. The survey itself will also produce quantitative information not previously seen on this scale.
It is envisaged that much of the survey will be completed by the end of 1997, the results of which shall be published on CD ROM and possibly video. Time and mode of publication may be dependent on postgraduate student thesis requirements. Follow-up observations at higher resolution are envisaged at optical, infrared and radio wavelengths.
This survey will be an important scientific resource and of significant value in the promotion of astronomy in the wider community.
| Next Section: Acknowledgements Title/Abstract Page: The MSSSO Wide Field Previous Section: Comparison with MOST Galactic | Contents Page: Volume 15, Number 1 |
© Copyright Astronomical Society of Australia 1997