作者
D Baade, K Meisenheimer, O Iwert, J Alonso, T Augusteijn, J Beletic, H Bellemann, W Benesch, A Böhm, H Böhnhardt, J Brewer, S Deiries, B Delabre, R Donaldson, C Dupuy, P Franke, R Gerdes, A Gilliotte, B Grimm, N Haddad, G Hess, G Ihle, R Klein, R Lenzen, J-L Lizon, D Mancini, N Münch, A Pizarro, P Prado, G Rahmer, J Reyes, F Richardson, E Robledo, F Sanchez, A Silber, P Sinclaire, R Wackermann, S Zaggia
发表日期
1999/3
期刊
Messenger, No. 95, p. 15-16, 19-21
卷号
95
页码范围
15-16
简介
The basic capabilities of the Wide Field Imager (WFI) were described in a previous Messenger article (No. 93, p. 13; see also Table 1) which also includes a brief account of the contributions by the three participating institutes, namely ESO (Garching and La Silla), the Max-Planck-Institut für Astronomie in Heidelberg, and the Osservatorio Astronomico di Capodimonte in Napoli. Table 1 summarises the most important characteristics. A first fairly complete version of the user manual is now offered via the WFI home page on the Web (URL: http://www. ls. eso. org/lasilla/Telescopes/2p2T/E2p2M/WFI/WFI. html). The same page also provides access to some examples of pictures obtained with the instrument. An exposure time calculator is available under the URL: http://www. eso. org/observing/etc/
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D Baade, K Meisenheimer, O Iwert, J Alonso… - Messenger, No. 95, p. 15-16, 19-21, 1999