|
|
Paper: |
Detecting Planets around Very Cool Stars at Near Infrared Wavelengths with the Radial Velocity Technique |
Volume: |
430, Pathways Towards Habitable Planets |
Page: |
526 |
Authors: |
Rodler, F.; del Burgo, C.; Martín, E. L.; Álvarez, C. |
Abstract: |
The radial velocity (RV) technique in the near-infrared is a powerful tool to search for low-mass planets around cool stars and sub-stellar objects. We investigate what precision can be achieved in RV measurements of an M9-dwarf in the Y-, J-, H-, and K-bands. Although late M-dwarfs emit the most flux in the J-band, we find that the highest RV-precision is attained in the Y-band. |
|
|
|
|