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Cross-correlation of the two micron galactic survey with IRAS

Published online by Cambridge University Press:  07 August 2017

T. Mahoney ,
F. Garzón ,
X. Calbet ,
P. Hammersley  and
M. J. Selby
T. Mahoney
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife (Spain)
F. Garzón
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife (Spain)
X. Calbet
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife (Spain)
P. Hammersley
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife (Spain)
M. J. Selby
Affiliation:
Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife (Spain)

Extract

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The Two Micron Galactic Survey (TMGS) is described by Calbet et al. (this symposium) and Mahoney et al. (1990). It has been cross-correlated with the IRAS point source catalogue (IRPS) using a 15-arcsec search radius, and preliminary results are presented here.

Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 309 - 310
Copyright
Copyright © Kluwer 1993 

References

Habing, H 1986, in Israel, F. P. (ed.), Light on Dark Matter. Proceedings of the First IRAS Conference, Noordwijk, The Netherlands. Dordrecht: Reidel.Google Scholar
Mahoney, T., Selby, M. J., Garzón, F., Hammersley, P. and Calbet, X. 1990, in Jarvis, B. J. and Terndrup, D. M. (eds.), Bulges of galaxies. ESO/CTIO workshop, La Serena, Chile.Google Scholar