Table 1.
Summary of the properties of the optical/NIR spectra.
| Instrument | N | λ range (Å) | R(λ/Δλ) |
|---|---|---|---|
| (1) | (2) | (3) | (4) |
| GTC/OSIRIS | 12 | 4800–10 000 | 587 |
| NOT/ALFOSC | 2 | 3200–9700 | 360 |
| 1 | 3650–7110 | 650 | |
| NTT/EFOSC2 | 2 | 4085–7520 | 370 |
| 1 | 3685–9315 | 210 | |
| SDSS/SDSS-I/II | 71 | 3800–9100 | 1850–2200 |
| SDSS/BOSS | 30 | 3600–10 400 | 1560–2560 |
| Subaru/FOCAS | 3 | 4700–9100 | 500 |
| TNG/DOLORES | 14 | 3000–8430 | 585 |
| UH88/WFGS | 1 | 3800–9700 | 440 |
| VLT/FORS2 | 12 | 4450–8650 | 440 |
| WHT/ACAM | 1 | 3300–9500 | 570 |
| WHT/ISIS | 15 | 5300–9300 | 844 |
| GTC/EMIR | 14 | 8500–13 500 | 987 |
| WHT/LIRIS | 1 | 9760–13 300 | 700 |
Notes. Column 1: name of the telescopes and instrumentes; Col. 2: number of spectra obtained with that instrument; Col. 3: wavelength coverage; Col. 4: resolution for a slit width of 1
, except for the WFGS and EMIR which are given for a slit of 1.1
. The two rows for NOT/ALFOSC and NTT/EFOSC2 correspond to different grism configurations. The last two rows correspond to NIR spectographs while the rest are for optical spectrographs.
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