Skip to main content Accessibility help
×
Home

Detectability of Earth-like Planets in Multi-Planet Systems: Preliminary Report

  • K. Goździewski, A. Niedzielski, J. Schneider, W. A. Traub (a1), C. Beichman (a2), A. F. Boden (a2), A. P. Boss (a3), S. Casertano (a4), J. Catanzarite (a1), D. Fischer (a5), E. B. Ford (a6), A. Gould (a7), S. Halverson (a8), A. Howard (a8), S. Ida (a9), N. J. Kasdin (a10), G. P. Laughlin (a11), H. F. Levison (a12), D. Lin (a11), V. Makarov (a2), J. Marr (a1), M. Muterspaugh (a13), S. N. Raymond (a14), D. Savransky (a10), M. Shao (a1), A. Sozzetti (a15) and C. Zhai (a1)...

Abstract


We ask if Earth-like planets (terrestrial mass and habitable-zone orbit) can be detected in multi-planet systems, using astrometric and radial velocity observations. We report here the preliminary results of double-blind calculations designed to answer this question.


Copyright

References

Hide All
[1] Cumming, A., Butler, R.P., Marcy, G.W., et al., 2008, PASP, 120, 531
[2] Gould, A., 2008 [arXiv:0807.4323], ApJ, submitted
[3] Scargle, J.D., 1982, ApJ, 263, 835

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed