High precision radial velocities in the near-infrared domain: Status and prospects

Bibcode
2011EPJWC..1602001M
DOI
10.1051/epjconf/20111602001
Martín, E. L.; Guenther, E.; Del Burgo, C.; Zapatero Osorio, M. R.; Deshpande, R.; Rodler, F.; Béjar, V. J. S.; Esparza, P.; Valdivielso, L.; Moitinho, A.; Amorim, A.; Lima, J.; Fiorenzano, A. M.; Magazzu, A.; Tata, R.
Bibliographical reference

Research, Science and Technology of Brown Dwarfs and Exoplanets: Proceedings of an International Conference held in Shangai on Occasion of a Total Eclipse of the Sun, Shangai, China, Edited by E.L. Martin; J. Ge; W. Lin; EPJ Web of Conferences, Volume 16, id.02001

Advertised on:
7
2011
Number of authors
15
IAC number of authors
4
Citations
0
Refereed citations
0
Description
The extension of the highly successful Doppler technique into the near-infrared (0.9-2.5 μm) is highly desirable as it would open the possibility for searches for extra-solar planets around young stars, very low-mass stars and brown dwarfs. Here we review the current status of this technique and discuss future prospects with particular emphasis on challenging problems for the next decade.
Type
Non-refereed

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