Free Access
Table 1
Spectroscopic stellar surveys for which distances were computed with our method.
| Survey | Year | Nstars | Spatial coverage | Typical S/N | λ range | R |
|
|
||||||
| SEGUE (DR9 G dwarfs) | 2004−2008 | ≃120 000 (35 000) | ≃1300 deg2 | 25 (35) | 0.38−0.92 μm | 2000 |
| APOGEE (DR10 HQ giants) | 2011−2014 | ≃100 000 (22 000) | ≃2800 deg2 | 100 (120) | 1.5−1.7 μm | 22 500 |
| RAVE (DR4 HQ giants) | 2006−2013 | ≃500 000 (9000) | ≃20 000 deg2 | 30 (70) | 0.84−0.88 μm | 7500 |
Notes. For each case we provide basic information, such as duration, number of stars for different signal-to-noise ratios (S/N), spatial and spectral coverage, and spectral resolving power.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.