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Table 1
Telescopes and instruments used for the confirmation of the Planck newly-discovered clusters at the Canary Islands observatories.
| Site | Telescope | Aperture [m] | Instrument | FoV | Pixel scale [′′] | Resolution | Nights |
|
|
|||||||
| OT, Tenerife ................ | IAC80 | 0.82 | CAMELOT |
|
0.304 | ... | 12 |
| ORM, La Palma ................ | NOT | 2.56 | ALFOSC | 7′ × 7′ | 0.188 | R = 550 | 0.5 |
| ORM, La Palma ................ | INT | 2.5 | WFC/IDS | 34′ × 34′ | 0.33 | R = 400 | 15 |
| ORM, La Palma ................ | TNG | 3.5 | DOLORES |
|
0.252 | R = 600 | 5 |
| ORM, La Palma ................ | WHT | 4.2 | ACAM | 8′ × 8′ | 0.253 | R = 400 | 2 |
| ORM, La Palma ................ | GTC | 10.4 | OSIRIS |
|
0.254 | R = 500 | 3 |
Notes. For spectroscopy, Col. 7 shows the resolution. Last column indicates the total number of clear nights (equivalent to 9 h) observed in each telescope for this work.
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