An activity catalogue of southern stars

被引:90
作者
Jenkins, J. S.
Jones, H. R. A.
Tinney, C. G.
Butler, R. P.
McCarthy, C.
Marcy, G. W.
Pinfield, D. J.
Carter, B. D.
Penny, A. J.
机构
[1] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
[2] Anglo Australian Observ, Epping, NSW 1710, Australia
[3] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA
[4] San Francisco State Univ, Dept Phys & Astron, San Francisco, CA 94132 USA
[5] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[6] Univ So Queensland, Fac Sci, Toowoomba, Qld 4350, Australia
[7] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
[8] SETI Inst, Mountain View, CA 94043 USA
[9] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
stars : activity; stars; low-mass; brown dwarfs; planetary systems; ultraviolet : stars;
D O I
10.1111/j.1365-2966.2006.10811.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have acquired high-resolution echelle spectra of 225 F6-M5 type stars in the Southern hemisphere. The stars are targets or candidates to be targets for the Anglo-Australian Planet Search. Ca II H& K line cores were used to derive activity indices for all of these objects. The indices were converted to the Mt. Wilson system of measurements and log R'(HK) values determined. A number of these stars had no previously derived activity indices. In addition, we have also included the stars from Tinney et al. using our Mt. Wilson calibration. The radial-velocity instability (also known as jitter) level was determined for all 21 planet-host stars in our data set. We find the jitter to be at a level considerably below the radial-velocity signatures in all but one of these systems. 19 stars from our sample were found to be active (logR'(HK) > -4.5) and thus have high levels of jitter. Radial-velocity analysis for planetary companions to these stars should proceed with caution.
引用
收藏
页码:163 / 173
页数:11
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