Abstract
We have completed observations for a new wide-field infrared survey. The survey covers a total area of 0.8 square degrees to a 5σ limiting magnitude of ~ 17.5 at K′ (2.1 μm) and ~ 18.5 at H (1.6 μm). We present preliininary results from this survey, including galaxy colours and luminosities.
also affiliated with the Anglo-Australian Observatory
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Broadhnrst, T. J., Ellis, R. S. and Shanks, T.: 1988, MNRAS 235, 827
Morton, D. C., Krug, P. A. and Tritton, K. P.: 1985, MNRAS 212, 325
Tritton, K. P. and Morton, D. C: 1984, MNRAS 209, 429
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1994 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Meadows, V.S., Allen, D.A. (1994). A New Wide-Field Infrared Survey Using Iris on the AAT. In: McLean, I.S. (eds) Infrared Astronomy with Arrays. Astrophysics and Space Science Library, vol 190. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1070-9_8
Download citation
DOI: https://doi.org/10.1007/978-94-011-1070-9_8
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4466-0
Online ISBN: 978-94-011-1070-9
eBook Packages: Springer Book Archive