Abstract
Several talks during this conference are based partly on infrared data obtained at ESO (Suntzeff et al., Danziger et al., Lucy et al., these proceedings). These data have been published by Bouchet et al. [1] and Bouchet et al. [2], and discussed, for instance, in Danziger et al. [3] and Lucy et al. [4]. Broad-band photometry from 1.2μm to 20μ, as well as narrow band photometry with a resolution of λ/△λ ~ 80 (CVF) have been obtained at ESO, La Silla, with the 3.60m, 2.2m and 1m telescopes, continuously since day 4 after outburst. Some higher resolution IR spectroscopy (λ/△λ ~ 1500) has also been obtained with the 3.6m telescope.
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References
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Bouchet, P., Danziger, I.J., Lucy, L.B. (1991). The ESO Infrared Data Set. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_5
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DOI: https://doi.org/10.1007/978-1-4612-2988-9_5
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