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Table 2

Observational circumstances.

Comet UT date r Δ Exptime Offset Slit Slit Seeing Seeing
(au) (km s-1) (au) (km s-1) (s) (′′) () (km × km) (′′) (km)

C/2002 T7 (LINEAR) 2004/05/06, 10:15 0.68 15.83 0.61 –65.62 1080 5 0.44 × 12.00 195 × 5 309 1.0 458
C/2002 T7 (LINEAR) 2004/05/26, 23:47 0.94 25.58 0.41 54.98 2678 0 0.30 × 12.00 89 × 3 568 0.7 198
C/2002 T7 (LINEAR) 2004/05/27, 01:06 0.94 25.59 0.42 55.20 1800 0 0.30 × 12.00 91 × 3 655 0.7 206
C/2002 T7 (LINEAR) 2004/05/28, 23:24 0.97 25.90 0.48 59.15 487 70 0.44 × 12.00 153 × 4 178 1.0 354
C/2002 T7 (LINEAR) 2004/05/29, 00:09 0.97 25.90 0.48 59.26 3600 70 0.44 × 12.00 153 × 4 178 1.0 205
73P-C SW 3 2006/05/27, 09:28 0.97 –4.17 0.15 12.31 4800 0 0.60 × 12.00 65 × 2 611 1.4 151
8P/Tuttle 2008/01/16, 01:00 1.04 –4.29 0.36 21.64 3600 0 0.44 × 10.00 115 × 1 305 1.0 261
8P/Tuttle 2008/01/28, 00:58 1.03 0.40 0.52 24.72 3900 0 0.44 × 10.00 166 × 3 771 0.9 319
8P/Tuttle 2008/02/04, 00:57 1.03 3.16 0.62 24.16 3900 0 0.44 × 10.00 198 × 4 497 1.0 450
103P/Hartley 2 2010/11/05, 07:18 1.06 2.53 0.16 7.08 2900 0 0.44 × 12.00 51 × 1 393 1.3 148
103P/Hartley 2 2010/11/05, 08:19 1.06 2.55 0.16 7.19 3200 0 0.44 × 12.00 57 × 1 567 1.8 205
103P/Hartley 2 2010/11/10, 07:17 1.07 4.05 0.18 7.96 2900 0 0.44 × 12.00 57 × 1 567 0.8 102
103P/Hartley 2 2010/11/10, 08:19 1.07 4.07 0.18 8.07 3200 0 0.44 × 12.00 51 × 1 393 0.8 97
103P/Hartley 2 2010/11/11, 05:53 1.08 4.33 0.19 7.94 4500 30 0.44 × 12.00 60 × 1 654 0.6 76
103P/Hartley 2 2010/11/11, 07:18 1.08 4.35 0.19 8.08 3600 20 0.44 × 12.00 60 × 1 654 0.6 81
103P/Hartley 2 2010/11/11, 08:16 1.08 4.36 0.19 8.19 2400 10 0.44 × 12.00 60 × 1 654 0.6 82
103P/Hartley 2 2010/11/11, 08:57 1.08 4.37 0.19 8.27 900 0 0.44 × 12.00 60 × 1 654 0.7 92

Notes. r is the heliocentric distance, Δ is the geocentric distance. and are the heliocentric and geocentric velocities. Exptime corresponds to the exposure time in seconds. Offset (arc seconds) corresponds to the distance between the slit and the center of the cometary nucleus. The slit-tail orientation provides the direction of the slit with respect to the cometary tail. Slit is the size of the entrance slit of the spectrograph in arc seconds. The next column gives the projected area covered by the slit. The last two columns present the seeing values in arc seconds and in km during the observations.

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