Telescope | Spectrograph | IFU | ![]() |
Ref. | Reduction tool/Pipeline | Ref. |
VLT/UT2 | GIRAFFE | FLAMES-ARGUS | 1 | 1 | BLDRS | 1a |
GIRAFFE PIPELINE | 1b | |||||
Gemini North/South | GMOS-N, GMOS-S | 3 | 2 | |||
Magellan I | IMACS | 8 | 3 | 3a | ||
WHT | WYFFOS | INTEGRAL | 1 | 4 | ||
Calar Alto 3.5 m | PMAS | LARR | 1 | 5 | P3D, P3D_ONLINE | 5a |
PPAK | 1 | 6 | PPAK_ONLINE | |||
AAT | AAOMEGA | SPIRAL | 2 | 7 | 2DFDR | 7a |
VLT/UT3 | VIMOS | VIMOS-IFU | 4 | 8 | VIPGI | 8a |
VIMOS PIPELINE | ||||||
McDonald 2.7 m | VIRUS-P | VIRUS-P | 1 | 9 | VACCINE | 9a |
Notes. In Col. 4 we specify the number of detectors of the IFU. Column 5 specifies the main instrument reference paper, and Col. 7 gives the reference of each instrument-specific reduction tool/pipeline.
References. 1 Avila et al. (2003);
Blecha et al. (2000);
Pasquini et al. (2000); 2 Allington-Smith et al. (2002); 3 Schmoll et al. (2004);
Bolton & Burles (2007); 4 Arribas et al. (1998); 5 Roth et al. (2005);
Becker (2002); 6 Kelz et al. (2006); 7 Smith et al. (2004);
Sharp et al. (2006); 8 LeFèvre et al. (2003);
Scodeggio et al. (2005); 9 Hill et al. (2008);
Adam et al., in prep.
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