Hostname: page-component-8448b6f56d-42gr6 Total loading time: 0 Render date: 2024-04-24T20:02:17.958Z Has data issue: false hasContentIssue false
  • English
  • Français

An Automatic Approach for Selecting New HA Emission-Line Galaxies

Published online by Cambridge University Press:  26 July 2016

O. Alonso ,
J. Zamorano ,
M. Rego ,
J. Gallego  and
A.G. Vitores
O. Alonso
Affiliation:
Dpto. de Astrofísica, Universidad Complutense de Madrid, 28040 Madrid, Spain
J. Zamorano
Affiliation:
Dpto. de Astrofísica, Universidad Complutense de Madrid, 28040 Madrid, Spain
M. Rego
Affiliation:
Dpto. de Astrofísica, Universidad Complutense de Madrid, 28040 Madrid, Spain
J. Gallego
Affiliation:
Dpto. de Astrofísica, Universidad Complutense de Madrid, 28040 Madrid, Spain
A.G. Vitores
Affiliation:
Dpto. de Astrofísica, Universidad Complutense de Madrid, 28040 Madrid, Spain

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The most unambiguous way to discover new emission-line galaxies (ELGs) is directly by the presence of their lines, using objective-prism plates of adequate resolution. The first survey using this technique was developed by Smith in 1975 with the 0.6 m CTIO Curtis Schmidt Telescope. The Universidad Complutense de Madrid (UCM) is carrying out a survey of ELGs with the Schmidt Telescope at Calar Alto (Almería, Spain) using the presence of Ha in emission in IIIa-F prism plates as selection criterion. The observational procedure and results are described in Rego et al. 1989; Zamorano et al. 1990; Zamorano et al. 1993.

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 611 - 614
Copyright
Copyright © Kluwer 1994 

References

Birkle, K., 1984. In ‘Astronomy with Schmidt-Type Telescopes’, ed. Capaccioli, M., IAU coll. 78, p. 203.Google Scholar
Borra, E.F., Edwards, G., Petrucci, F., Beauchemin, M., Brousseau, D., Grondin, L. and Beaulieu, A., 1987. Publ. Astron. Soc. Pacific, 99, 535.CrossRefGoogle Scholar
Guibert, J. and Moreau, O., 1991. The Messenger, 64, 69.Google Scholar
Moreau, O., 1992. PhD Thesis, Université de Paris 7.Google Scholar
Paturel, G., Fouqué, P., Bottinelli, L. Gouguenheim, L., 1989. Astron. Astrophys. Suppl., 80, 299.Google Scholar
Rego, M., Zamorano, J and Gonzalez-Riestra, R., 1989. Astron. Astrophys. Suppl., 79, 443.Google Scholar
Smith, M.G., 1975. Astrophys. J., 202, 591.CrossRefGoogle Scholar
Zamorano, J., Rego, M., Gonzalez-Riestra, R. and Rodríguez, G., 1990. Astrophys. Space Sci., 170, 353.CrossRefGoogle Scholar
Zamorano, J., Rego, M., Gallego, J., Vitores, A.G., Gonzalez-Riestra, R. and Rodríguez-Caderot, G., 1993. Astrophys. J. Suppl., submitted.Google Scholar