Table 1
Anticentre sample of kinematically selected thin disc RRL stars.
| Source ID | d (kpc) | ∆d (kpc) | l (deg) | b (deg) | μl (µas/yr) | μb (µas/yr) | [Fe/H] (dex) | P (days) | AmpV (mag) | F |
|---|---|---|---|---|---|---|---|---|---|---|
| 51220203721624064 | 3.39 | 0.14 | 170.018375 | –25.580921 | 3.2322 | –0.5654 | –0.47 | 0.481201 | 0.84 | 0 |
| 72425797289881344 | 2.55 | 0.13 | 152.701939 | –47.293983 | 2.7634 | –0.8368 | –0.35 | 0.28662 | 0.21 | 0 |
| 80556926295542528 | 1.63 | 0.08 | 149.994094 | –40.849758 | 3.3490 | –8.9908 | –0.63 | 0.354279 | 0.40 | 0 |
Notes. Description of the columns: Gaia DR3 source ID, distance (d), distance error (∆d), Galactic longitude (l) and latitude (b), proper motion in l (μl) and b (μb), the metallicity adopted for the distance calculation ([Fe∕H]), the period (P), V-band amplitude (AmpV), and the value “F” is 1 when the metallicity adopted is the photometric one and 0 if it was assigned (see Sect. 2). The first few rows of the table are shown to provide guidance regarding its form and content. The full version of the table is available in the CDS.
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.