Table D.1
Fitted Serkowski parameters, with the polarization angle, for the field stars used to derive the interstellar polarization of o Aquarii.
| Star | RA (J2000) | Dec (J2000) | Pmax (%) | λmax (μm) | ⟨PAIS⟩ (deg) |
|---|---|---|---|---|---|
| (hh:mm:ss) | (deg:arcmin:arcsec) | ||||
| HD 208719 | 21 58 20.0 | −01 49 46.7 |  |
 |
130.7 ± 2.9 |
| HD 209348 | 22 02 48.4 | −02 28 44.4 |  |
 |
128 ± 44 |
| 2MASS J22025363-0229207 | 22 02 53.6 | −02 29 20.7 |  |
 |
135.4 ± 9.1 |
| 2MASS J22025544-0230058 | 22 02 55.4 | −02 30 05.8 |  |
 |
136.8 ± 0.6 |
Notes. We show the median and the 15.87th and 84.13th percentiles for Pmax and λmax from the MCMC analysis (more details in Bednarski 2016). The interstellar polarization angle estimated for each field star is the mean value among the observations in the BVRI-bands (⟨PAIS ⟩).
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.