Log of observations of the HD 72106 system obtained with ESPaDOnS. Integration times refer to the complete set of four subexposures used to produce each Stokes V spectrum (Donati et al. 1997). Peak S/N values are reported for the original reduced spectra with 1.8 km s−1 spectral pixels. Magnetic measurements for combined observations refer to results for the reconstructed spectra of the primary. The letter D in the LSD detection column indicates that the Stokes V LSD profile is inconsistent with the null field hypothesis at the 99.999 per cent confidence limit, indicating the presence of a magnetic field. The letter N indicates that the inconsistency was at the 99.9 per cent limit or less, and hence cannot be take as strong evidence for the detection of a magnetic field. The letters MD indicate a ‘marginal’ detection, with a value between 99.9 and 99.999 per cent, and are considered suggestive of a magnetic field, but not conclusive. (Donati, Semel & Rees 1992; Donati et al. 1997). Note that the observation from 2005 February was first published by Wade et al. (2005).
ut date | HJD (−245 0000) | Component (HD 72106) | Integration time (s) | Peak S/N I | Bz (G) | LSD detection |
2005 February 22 | 3423.9248 | A and B | 2400 | 201 | 228 ± 50 | D |
2006 January 09 | 3745.029 67 | A and B | 2400 | 219 | 345 ± 42 | D |
2006 January 11 | 3747.020 34 | A and B | 3200 | 143 | 261 ± 76 | MD |
2006 January 12 | 3747.996 29 | A | 1200 | 149 | −13 ± 44 | MD |
2006 January 12 | 3748.014 96 | B | 1200 | 76 | 2 ± 168 | N |
2006 February 11 | 3777.878 60 | A and B | 2000 | 238 | 231 ± 40 | D |
2006 February 11 | 3777.951 49 | A and B | 2400 | 253 | 124 ± 37 | D |
2006 February 12 | 3778.861 72 | A and B | 2400 | 282 | 282 ± 34 | D |
2006 February 13 | 3779.872 02 | A and B | 2400 | 184 | 170 ± 53 | D |
2006 February 13 | 3779.981 27 | A and B | 2400 | 128 | 157 ± 156 | N |
2007 March 02 | 4161.772 82 | A and B | 2400 | 254 | 350 ± 36 | D |
2007 March 02 | 4161.802 56 | A and B | 2400 | 265 | 297 ± 34 | D |
2007 March 02 | 4161.902 82 | A and B | 2400 | 297 | 214 ± 30 | D |
2007 March 03 | 4162.857 13 | A and B | 2400 | 208 | 246 ± 44 | D |
2007 March 04 | 4163.835 61 | A and B | 2400 | 322 | 202 ± 27 | D |
2007 March 05 | 4164.846 50 | B | 3200 | 209 | −51 ± 55 | N |
2007 March 05 | 4164.883 87 | A | 2400 | 248 | 320 ± 23 | D |
2007 March 05 | 4164.909 61 | A and B | 1600 | 277 | 374 ± 32 | D |
2007 March 09 | 4168.857 91 | A and B | 2400 | 283 | 304 ± 33 | D |
2007 March 09 | 4168.909 47 | A and B | 2400 | 272 | 252 ± 34 | D |
ut date | HJD (−245 0000) | Component (HD 72106) | Integration time (s) | Peak S/N I | Bz (G) | LSD detection |
2005 February 22 | 3423.9248 | A and B | 2400 | 201 | 228 ± 50 | D |
2006 January 09 | 3745.029 67 | A and B | 2400 | 219 | 345 ± 42 | D |
2006 January 11 | 3747.020 34 | A and B | 3200 | 143 | 261 ± 76 | MD |
2006 January 12 | 3747.996 29 | A | 1200 | 149 | −13 ± 44 | MD |
2006 January 12 | 3748.014 96 | B | 1200 | 76 | 2 ± 168 | N |
2006 February 11 | 3777.878 60 | A and B | 2000 | 238 | 231 ± 40 | D |
2006 February 11 | 3777.951 49 | A and B | 2400 | 253 | 124 ± 37 | D |
2006 February 12 | 3778.861 72 | A and B | 2400 | 282 | 282 ± 34 | D |
2006 February 13 | 3779.872 02 | A and B | 2400 | 184 | 170 ± 53 | D |
2006 February 13 | 3779.981 27 | A and B | 2400 | 128 | 157 ± 156 | N |
2007 March 02 | 4161.772 82 | A and B | 2400 | 254 | 350 ± 36 | D |
2007 March 02 | 4161.802 56 | A and B | 2400 | 265 | 297 ± 34 | D |
2007 March 02 | 4161.902 82 | A and B | 2400 | 297 | 214 ± 30 | D |
2007 March 03 | 4162.857 13 | A and B | 2400 | 208 | 246 ± 44 | D |
2007 March 04 | 4163.835 61 | A and B | 2400 | 322 | 202 ± 27 | D |
2007 March 05 | 4164.846 50 | B | 3200 | 209 | −51 ± 55 | N |
2007 March 05 | 4164.883 87 | A | 2400 | 248 | 320 ± 23 | D |
2007 March 05 | 4164.909 61 | A and B | 1600 | 277 | 374 ± 32 | D |
2007 March 09 | 4168.857 91 | A and B | 2400 | 283 | 304 ± 33 | D |
2007 March 09 | 4168.909 47 | A and B | 2400 | 272 | 252 ± 34 | D |
Log of observations of the HD 72106 system obtained with ESPaDOnS. Integration times refer to the complete set of four subexposures used to produce each Stokes V spectrum (Donati et al. 1997). Peak S/N values are reported for the original reduced spectra with 1.8 km s−1 spectral pixels. Magnetic measurements for combined observations refer to results for the reconstructed spectra of the primary. The letter D in the LSD detection column indicates that the Stokes V LSD profile is inconsistent with the null field hypothesis at the 99.999 per cent confidence limit, indicating the presence of a magnetic field. The letter N indicates that the inconsistency was at the 99.9 per cent limit or less, and hence cannot be take as strong evidence for the detection of a magnetic field. The letters MD indicate a ‘marginal’ detection, with a value between 99.9 and 99.999 per cent, and are considered suggestive of a magnetic field, but not conclusive. (Donati, Semel & Rees 1992; Donati et al. 1997). Note that the observation from 2005 February was first published by Wade et al. (2005).
ut date | HJD (−245 0000) | Component (HD 72106) | Integration time (s) | Peak S/N I | Bz (G) | LSD detection |
2005 February 22 | 3423.9248 | A and B | 2400 | 201 | 228 ± 50 | D |
2006 January 09 | 3745.029 67 | A and B | 2400 | 219 | 345 ± 42 | D |
2006 January 11 | 3747.020 34 | A and B | 3200 | 143 | 261 ± 76 | MD |
2006 January 12 | 3747.996 29 | A | 1200 | 149 | −13 ± 44 | MD |
2006 January 12 | 3748.014 96 | B | 1200 | 76 | 2 ± 168 | N |
2006 February 11 | 3777.878 60 | A and B | 2000 | 238 | 231 ± 40 | D |
2006 February 11 | 3777.951 49 | A and B | 2400 | 253 | 124 ± 37 | D |
2006 February 12 | 3778.861 72 | A and B | 2400 | 282 | 282 ± 34 | D |
2006 February 13 | 3779.872 02 | A and B | 2400 | 184 | 170 ± 53 | D |
2006 February 13 | 3779.981 27 | A and B | 2400 | 128 | 157 ± 156 | N |
2007 March 02 | 4161.772 82 | A and B | 2400 | 254 | 350 ± 36 | D |
2007 March 02 | 4161.802 56 | A and B | 2400 | 265 | 297 ± 34 | D |
2007 March 02 | 4161.902 82 | A and B | 2400 | 297 | 214 ± 30 | D |
2007 March 03 | 4162.857 13 | A and B | 2400 | 208 | 246 ± 44 | D |
2007 March 04 | 4163.835 61 | A and B | 2400 | 322 | 202 ± 27 | D |
2007 March 05 | 4164.846 50 | B | 3200 | 209 | −51 ± 55 | N |
2007 March 05 | 4164.883 87 | A | 2400 | 248 | 320 ± 23 | D |
2007 March 05 | 4164.909 61 | A and B | 1600 | 277 | 374 ± 32 | D |
2007 March 09 | 4168.857 91 | A and B | 2400 | 283 | 304 ± 33 | D |
2007 March 09 | 4168.909 47 | A and B | 2400 | 272 | 252 ± 34 | D |
ut date | HJD (−245 0000) | Component (HD 72106) | Integration time (s) | Peak S/N I | Bz (G) | LSD detection |
2005 February 22 | 3423.9248 | A and B | 2400 | 201 | 228 ± 50 | D |
2006 January 09 | 3745.029 67 | A and B | 2400 | 219 | 345 ± 42 | D |
2006 January 11 | 3747.020 34 | A and B | 3200 | 143 | 261 ± 76 | MD |
2006 January 12 | 3747.996 29 | A | 1200 | 149 | −13 ± 44 | MD |
2006 January 12 | 3748.014 96 | B | 1200 | 76 | 2 ± 168 | N |
2006 February 11 | 3777.878 60 | A and B | 2000 | 238 | 231 ± 40 | D |
2006 February 11 | 3777.951 49 | A and B | 2400 | 253 | 124 ± 37 | D |
2006 February 12 | 3778.861 72 | A and B | 2400 | 282 | 282 ± 34 | D |
2006 February 13 | 3779.872 02 | A and B | 2400 | 184 | 170 ± 53 | D |
2006 February 13 | 3779.981 27 | A and B | 2400 | 128 | 157 ± 156 | N |
2007 March 02 | 4161.772 82 | A and B | 2400 | 254 | 350 ± 36 | D |
2007 March 02 | 4161.802 56 | A and B | 2400 | 265 | 297 ± 34 | D |
2007 March 02 | 4161.902 82 | A and B | 2400 | 297 | 214 ± 30 | D |
2007 March 03 | 4162.857 13 | A and B | 2400 | 208 | 246 ± 44 | D |
2007 March 04 | 4163.835 61 | A and B | 2400 | 322 | 202 ± 27 | D |
2007 March 05 | 4164.846 50 | B | 3200 | 209 | −51 ± 55 | N |
2007 March 05 | 4164.883 87 | A | 2400 | 248 | 320 ± 23 | D |
2007 March 05 | 4164.909 61 | A and B | 1600 | 277 | 374 ± 32 | D |
2007 March 09 | 4168.857 91 | A and B | 2400 | 283 | 304 ± 33 | D |
2007 March 09 | 4168.909 47 | A and B | 2400 | 272 | 252 ± 34 | D |
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