Astron. Astrophys. 323, 235-242 (1997)

Acknowledgements

Data from the IRIS network depends on the coordinated efforts of many peoples from several nations. The authors wish to thank those who have conceived the instrument: E. Fossat and G. Grec; those who have contributed to build and maintain all instruments on site: B. Gelly, J.F. Manigault, G. Rouget, J. Demarcq, G. Galou, A. Escobar, J.M. Robillot; those who have operated the observing sites: M. Baijumamov, S. Ehgamberdiev, S. Ilyasov, S. Khalikov, I. Khamitov, G. Menshikov, S. Raubaev, J.T. Hoeksema, Z. Benkhaldoun, M. Lazrek, S. Kadiri, H. Touma, M. Anguera, A. Jimenez, P.L. Palle, A. Pimienta, C. Regulo, T. Roca Cortes, L. Sanchez, F.X. Schmider; R. Luckhurst, those who have developed the analysis software: S. Ehgamberdiev, S. Khalikov, E. Fossat, B. Gelly, M. Lazrek, P.L. Palle, L. Sanchez, E. Gavryuseva, V. Gavryusev; and those who have contributed to the success of the IRIS project in other critical ways: P. Delache, D. Gough, I. Roxburgh, F. Hill, T. Roca-Cortes, G. Zatsepin, T. Yuldashbaev, L. Woltjer, H. Van der Laan, D. Hofstadt, J. Kennewell, D. Cole, P. Scherrer, F. Sanchez, J.P. Veziant and the Birmingham University Solar Network for sharing the observational facility in Tenerife.
We wish to thank Steve Tomczyk and Jesper Schou in making available to us the LOWL frequency tables.
The IRIS network was funded and is supported by the Institut National des Sciences de l'Univers (INSU) and the Centre National de la Recherche Scientifique (CNRS).

© European Southern Observatory (ESO) 1997

Online publication: June 5, 1998

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