Table 1

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 dateHJD (−245 0000)Component (HD 72106)Integration time (s)Peak S/N IBz (G)LSD detection
2005 February 223423.9248A and B2400201228 ± 50D
2006 January 093745.029 67A and B2400219345 ± 42D
2006 January 113747.020 34A and B3200143261 ± 76MD
2006 January 123747.996 29A1200149−13 ± 44MD
2006 January 123748.014 96B1200762 ± 168N
2006 February 113777.878 60A and B2000238231 ± 40D
2006 February 113777.951 49A and B2400253124 ± 37D
2006 February 123778.861 72A and B2400282282 ± 34D
2006 February 133779.872 02A and B2400184170 ± 53D
2006 February 133779.981 27A and B2400128157 ± 156N
2007 March 024161.772 82A and B2400254350 ± 36D
2007 March 024161.802 56A and B2400265297 ± 34D
2007 March 024161.902 82A and B2400297214 ± 30D
2007 March 034162.857 13A and B2400208246 ± 44D
2007 March 044163.835 61A and B2400322202 ± 27D
2007 March 054164.846 50B3200209−51 ± 55N
2007 March 054164.883 87A2400248320 ± 23D
2007 March 054164.909 61A and B1600277374 ± 32D
2007 March 094168.857 91A and B2400283304 ± 33D
2007 March 094168.909 47A and B2400272252 ± 34D
ut dateHJD (−245 0000)Component (HD 72106)Integration time (s)Peak S/N IBz (G)LSD detection
2005 February 223423.9248A and B2400201228 ± 50D
2006 January 093745.029 67A and B2400219345 ± 42D
2006 January 113747.020 34A and B3200143261 ± 76MD
2006 January 123747.996 29A1200149−13 ± 44MD
2006 January 123748.014 96B1200762 ± 168N
2006 February 113777.878 60A and B2000238231 ± 40D
2006 February 113777.951 49A and B2400253124 ± 37D
2006 February 123778.861 72A and B2400282282 ± 34D
2006 February 133779.872 02A and B2400184170 ± 53D
2006 February 133779.981 27A and B2400128157 ± 156N
2007 March 024161.772 82A and B2400254350 ± 36D
2007 March 024161.802 56A and B2400265297 ± 34D
2007 March 024161.902 82A and B2400297214 ± 30D
2007 March 034162.857 13A and B2400208246 ± 44D
2007 March 044163.835 61A and B2400322202 ± 27D
2007 March 054164.846 50B3200209−51 ± 55N
2007 March 054164.883 87A2400248320 ± 23D
2007 March 054164.909 61A and B1600277374 ± 32D
2007 March 094168.857 91A and B2400283304 ± 33D
2007 March 094168.909 47A and B2400272252 ± 34D
Table 1

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 dateHJD (−245 0000)Component (HD 72106)Integration time (s)Peak S/N IBz (G)LSD detection
2005 February 223423.9248A and B2400201228 ± 50D
2006 January 093745.029 67A and B2400219345 ± 42D
2006 January 113747.020 34A and B3200143261 ± 76MD
2006 January 123747.996 29A1200149−13 ± 44MD
2006 January 123748.014 96B1200762 ± 168N
2006 February 113777.878 60A and B2000238231 ± 40D
2006 February 113777.951 49A and B2400253124 ± 37D
2006 February 123778.861 72A and B2400282282 ± 34D
2006 February 133779.872 02A and B2400184170 ± 53D
2006 February 133779.981 27A and B2400128157 ± 156N
2007 March 024161.772 82A and B2400254350 ± 36D
2007 March 024161.802 56A and B2400265297 ± 34D
2007 March 024161.902 82A and B2400297214 ± 30D
2007 March 034162.857 13A and B2400208246 ± 44D
2007 March 044163.835 61A and B2400322202 ± 27D
2007 March 054164.846 50B3200209−51 ± 55N
2007 March 054164.883 87A2400248320 ± 23D
2007 March 054164.909 61A and B1600277374 ± 32D
2007 March 094168.857 91A and B2400283304 ± 33D
2007 March 094168.909 47A and B2400272252 ± 34D
ut dateHJD (−245 0000)Component (HD 72106)Integration time (s)Peak S/N IBz (G)LSD detection
2005 February 223423.9248A and B2400201228 ± 50D
2006 January 093745.029 67A and B2400219345 ± 42D
2006 January 113747.020 34A and B3200143261 ± 76MD
2006 January 123747.996 29A1200149−13 ± 44MD
2006 January 123748.014 96B1200762 ± 168N
2006 February 113777.878 60A and B2000238231 ± 40D
2006 February 113777.951 49A and B2400253124 ± 37D
2006 February 123778.861 72A and B2400282282 ± 34D
2006 February 133779.872 02A and B2400184170 ± 53D
2006 February 133779.981 27A and B2400128157 ± 156N
2007 March 024161.772 82A and B2400254350 ± 36D
2007 March 024161.802 56A and B2400265297 ± 34D
2007 March 024161.902 82A and B2400297214 ± 30D
2007 March 034162.857 13A and B2400208246 ± 44D
2007 March 044163.835 61A and B2400322202 ± 27D
2007 March 054164.846 50B3200209−51 ± 55N
2007 March 054164.883 87A2400248320 ± 23D
2007 March 054164.909 61A and B1600277374 ± 32D
2007 March 094168.857 91A and B2400283304 ± 33D
2007 March 094168.909 47A and B2400272252 ± 34D
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