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- 10 Apr. 09: RV measurements with amateur spectrograph (Christian Buil).
- 10 sep. 03: New upper limit of 0.39 for the reflection albedo (Leigh et al 2003)
- 20 apr. 03: Planet in wide (a ~ 240 AU) binary system (Eggenberger et al 2003)
- 22 spt. 2000: the planet
not so bright as
previously announced (Cameron et al).
- Exhibits coherent variations in residual velocities
consistent with additional companion.
24 Jul. 00: the source of RV variation remains speculative, depending on completion of one full orbit (Fischer et al 2000).
- `Probable detection' of the reflected star-light by the planet (Cameron et. al, 1999). The albedo is claimed to be detected only from 456 to 524 nm.
- The star has a companion ( GJ 527B) about 240 AU away.
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