Table 2: Log of the observations in spectral regions containing photospheric lines.

Date
HJD Phase Lines RV $\pm \sigma$(RV) Observa- Spectro-
  2 400 000+     km s-1 km s-1 tory graph

07.06.95
49 875.590 0.40 He I 5016, 5048 +4.0 0.4 OHP ÉLODIE
      S II 5606, 5647 +5.7 2.1    

09.07.97
50 638.525 0.97 He I 5016, 5048 -8.5 0.6 OHP ÉLODIE
      S II 5606, 5647 -7.2 0.5    

16.11.00
51 864.600 0.88 He I 4009, 4026 -21.0 3.0 SAO MSS
      Si II 4128, 4131 -9.0 1.0    

11.06.01
52 072.300 0.06 S II 5606, 5647 -1.4 0.8 SAO PFES

12.10.01
52 194.741 0.14 S II 5606, 5647 -1.6 1.0 McD Sandiford

29.11.01
52 242.647 0.17 S II 5606, 5647 +2.9 0.2 SAO LYNX

06.12.01
52 250.300 0.17 He I 4009, 4026 +15.0 3.0 SAO MSS
      Si II 4128, 4131 +17.0 5.0    

27.04.02
52 391.510 0.28 He I 5016, 5048 -3.0 0.2 SAO NES
      S II 5606, 5647 -4.7 0.8    

28.05.02
52 423.296 0.31 S II 5606, 5647 -1.7 3.0 SAO LYNX

12.07.02
52 467.500 0.33 He I 4009, 4026 +4.0 2.0 CFHT Gecko

26.07.02
52 482.233 0.34 He I 5016, 5048 -4.2 0.8 SAO NES
      S II 5606, 5647 -0.6 0.7    

25.09.02
52 542.665 0.40 S II 5606, 5647 -2.1 3.0 McD Sandiford
      S II 5453        
The observational data are presented in the following columns: (1) - the observing date (DD.MM.YY); (2) - the heliocentric Julian date; (3) - the phase of the 1345d-period of activity calculated according to the ephemeris of Miroshnichenko et al. (1998); (4) - the photospheric lines whose radial velocities were measured; (5) and (6) - the mean radial velocity for a given element and its error, respectively; (7) - the observatory where the data were obtained; (8) - the spectrograph which was used to obtain the spectrum.

Source LaTeX | All tables | In the text