Table E.1
Hot star candidates with proper motion measurement.
| Source name | pml | σ pml | pmb | σ pmb | H - KS | xoffset | yoffset |
|---|---|---|---|---|---|---|---|
| [mas· yr−1] | [mas· yr−1 ] | [mas· yr−1] | [mas· yr−1] | [mag] | [arcsec] | [arcsec] | |
| F2_26630347-29161867_Ks12.97 | -7.57976 | 0.43751 | -0.65124 | 0.37540 | 1.93 | -659.12 | 15.16 |
| F2_26636584-29096720_Ks12.81 | -4.31695 | 0.49181 | 0.43328 | 0.46925 | 1.77 | -356.72 | -29.87 |
| F2_26639297-29048702_Ks13.22 | -3.29715 | 0.44726 | -2.12941 | 0.65878 | 1.97 | -164.70 | -12.62 |
| F2_26640100-29016754_Ks12.85 | -6.95449 | 0.46801 | -3.79296 | 0.46173 | 1.53 | -53.37 | 25.74 |
| F2_26641345-29012257_Ks13.11 | 5.26893 | 0.81193 | 4.58466 | 0.65169 | 1.77 | -19.13 | 0.72 |
| F2_26640979-29010162_Ks12.83 | 2.51382 | 0.37853 | -2.41210 | 0.41530 | 2.33 | -18.69 | 14.48 |
| F2_26641458-29010031_Ks11.83 | -6.07076 | 1.10348 | -1.46760 | 0.93555 | 1.74 | -10.43 | 1.85 |
| F2_26641415-29009539_Ks12.13 | -4.05693 | 0.98551 | 3.53581 | 0.83244 | 1.69 | -9.63 | 3.93 |
| F2_26641397-29009415_Ks10.90 | -0.65542 | 0.99264 | -6.00427 | 0.89523 | 1.87 | -9.54 | 4.65 |
| F2_26641885-29006378_Ks10.15 | 3.35352 | 0.44717 | 6.32263 | 0.56343 | 3.24 | 7.80 | -2.77 |
| F2_26641107-28999369_Ks11.50 | 3.10693 | 0.37106 | -0.54336 | 0.35236 | 1.88 | 16.57 | 31.28 |
| F2_26642368-29002531_Ks12.29 | -1.91629 | 0.55541 | 0.04954 | 0.52567 | 1.97 | 27.54 | -8.54 |
| F2_26640643-28988766_Ks11.85 | 2.08185 | 0.50043 | 3.29429 | 0.45478 | 1.37 | 41.54 | 63.64 |
| F2_26643866-28966084_Ks12.46 | 0.42095 | 0.37018 | 1.33551 | 0.34400 | 1.41 | 164.12 | 19.53 |
| F2_26650085-28895227_Ks12.15 | 2.76172 | 0.38619 | -0.99954 | 0.29024 | 1.42 | 483.92 | -14.98 |
| F2_26652917-28857695_Ks12.95 | -6.01836 | 0.43309 | 3.70225 | 0.34873 | 2.03 | 645.75 | -20.93 |
| F2_26652484-28854546_Ks12.20 | -2.00436 | 0.38303 | 8.36375 | 0.41923 | 1.34 | 648.33 | -3.38 |
| F2_26653299-28843451_Ks11.39 | 5.23811 | 0.51540 | 1.14242 | 0.50952 | 1.51 | 695.81 | -4.55 |
| F2_26652979-28836376_Ks12.48 | 1.01451 | 0.33587 | 0.40466 | 0.30085 | 1.42 | 712.32 | 17.32 |
| F2_26654034-28827679_Ks11.74 | -1.56756 | 0.33822 | -0.16292 | 0.38063 | 1.64 | 756.36 | 5.18 |
| F2_26654547-28825665_Ks11.71 | 2.05280 | 0.37501 | -1.13780 | 0.65325 | 1.66 | 770.97 | -4.87 |
| F2_26654773-28826262_Ks12.68 | 2.58119 | 0.48971 | -1.26814 | 0.66280 | 1.60 | 772.84 | -12.07 |
| F2_26654877-28813469_Ks12.39 | -3.82819 | 0.68378 | 1.27034 | 0.40760 | 1.63 | 813.89 | 9.08 |
Notes. The columns denote the source name, proper motion from Shahzamanian et al. (2022) along Galactic longitude l, associated uncertainty, proper motion along Galactic latitude b, associated uncertainty, colour H - KS, and the offset coordinates from Sgr A*, as shown in Fig. 7.
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.