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Table 2:

Observing run details.

Id.
Date Telescope Instrument CCD chip Spectral range Orders Dispersion FWHM
          (Å)   (Å) (Å)

1
1999 Jul. 24-29 2.2 ma FOCES1 2048 $\times$ 2048 15 $\mu$m LORAL#11 3910-9075 84 0.03-0.07 0.09-0.15
2 1999 Nov. 26-27 NOTb SOFIN2 1152 $\times$ 770 EEV P88200 3525-10 425 44 0.06-0.17 0.14-0.32
3 2000 Jan. 18-22 INTc MUSICOS3 1024 $\times$ 1024 24 $\mu$m TEK5 4430-10 225 73 0.07-0.15 0.16-0.30
4 2000 Aug. 05-11 INTc MUSICOS3 1024 $\times$ 1024 24 $\mu$m TEK5 4430-10 225 73 0.07-0.15 0.16-0.30
5 2000 Nov. 10-13 NOTb SOFIN2 1152 $\times$ 770 EEV P88200 3525-10 425 44 0.06-0.17 0.14-0.32
6 2001 Apr. 02-05 INTc IDS4 2148 $\times$ 4200 13.5 $\mu$m EEV10a 3554-7137 1 0.48 1.22
7 2001 Sep. 21-24 2.2 ma FOCES1 2048 $\times$ 2048 24 $\mu$m Site#1d 3510-10 700 112 0.04-0.13 0.08-0.35
8 2001 Oct. 10-11 TNGd SARG5 2(2048 $\times$ 4096) 13.5 $\mu$m EEV 4280 4960-10 110 62 0.02-0.04 0.08-0.17
9 2001 Dec. 19- HETe HRS6 2(2048 $\times$ 4096) 15 $\mu$m Marconi 5040-8775 52 0.06-0.11 0.15-0.28
  2002 Feb. 28              
10 2002 Apr. 22-25 2.2 ma FOCES1 2048 $\times$ 2048 24 $\mu$m Site#1d 3510-10 700 112 0.04-0.13 0.08-0.35
11 2002 Jul. 01-06 2.2 ma FOCES1 2048 $\times$ 2048 24 $\mu$m Site#1d 3510-10 700 112 0.04-0.13 0.08-0.35
12 2002 Aug. 21-29 NOTb SOFIN2 2048 $\times$ 2048 2K3EB PISKUNOV1 3525-10 200 42 0.02-0.05 0.05-0.15

Notes. (a) 2.2 m telescope at German Spanish Astronomical Observatory (CAHA) (Almería, Spain); (b) 2.56 m Nordic Optical Telescope (NOT) at Observatorio del Roque de los Muchachos (La Palma, Spain); (c) 2.5 m Isaac Newton Telescope (INT) at Observatorio del Roque de los Muchachos (La Palma, Spain); (d) 3.5 m Telescopio Nazionale Galileo (TNG) at Observatorio del Roque de los Muchachos (La Palma, Spain); (e) 9.2 m Hobby-Eberly Telescope (HET) at McDonald Observatory (Texas, USA).
(1) FOCES: Fiber Optics Cassegrain Echelle Spectrograph; (2) SOFIN: Soviet Finnish High Resolution Echelle Spectrograph; (3) MUSICOS: spectrograph developed as part of MUlti-SIte COntinuous Spectroscopy project; (4) IDS: Intermediate Dispersion Spectrograph; (5) SARG: Spettrografo di Alta Resoluzione Galileo; (6) HRS: High Resolution Spectrograph.


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