Table 4
Program stars: ID, spectroscopy, photometry.
| # | Star | Instrument | S/N | Photometry | Remark |
|
|
|||||
| 1 | HD 35299 | Fiesa | 250 | (1), (3), (4), (5) | single |
| 2 | HD 35912 | Fiesa | 240 | (1), (3), (4), (5) | single |
| 3 | HD 37042 | Fiesa | 205 | (2), (3), (4) | single |
| 4 a | HD 75821 | Feros | 350 | (1), (3), (4), (5) | SB2 |
| 4 b | HD 75821 | Feros | 340 | (1), (3), (4), (5) | SB2 |
| 4 c | HD 75821 | Feros | 340 | (1), (3), (4), (5) | SB2 |
| 5 | HD 119109 | Feros | 220 | (1), (4), (5) | SB2 |
| 6 | HD 213420 | Fies | 350 | (1), (3), (4), (5) | SB2 |
Notes. The fourth column is the mean S/N of the spectrum obtained with one of the two high-resolution spectrographs Fies (λ/ Δλ = 45 000, Frandsen & Lindberg 1999) or Feros (λ/ Δλ = 48 000, Kaufer et al. 1999).
Spectra have been taken from the IACOB database (Simón-Díaz et al. 2011a) by courtesy of S. Simón-Díaz and were first presented and analyzed in Simón-Díaz (2010).
Reference. (1) Mermilliod (1991); (2) Ducati (2002); (3) Hauck & Mermilliod (1998); (4) Høg et al. (2000); (5) van Leeuwen (2007).
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.