Open Access

Table E.2

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_26628195-29192692_Ks12.37 5.24955 0.13227 -1.19721 0.17863 0.13 -789.08 14.95
F2_26629854-29181913_Ks11.79 -2.53096 0.19062 -0.57642 0.23858 0.10 -728.75 -9.30
F2_26630038-29173820_Ks11.47 -2.44452 0.50339 -1.32795 0.48355 0.26 -700.89 0.99
F2_26630347-29161867_Ks12.97 -9.35104 0.33850 -0.23914 0.39156 1.93 -659.12 15.16
F2_26648660-28902523_Ks11.00 -1.56492 1.69571 -0.06578 1.29770 0.36 438.12 9.70
F2_26648845-28894819_Ks9.96 -1.75364 0.67338 -0.13754 0.89820 1.15 464.85 19.13
F2_26650085-28895227_Ks12.15 -4.50275 0.39608 -1.08558 0.35254 1.42 483.92 -14.98
F2_26649948-28885368_Ks11.78 -1.64393 1.77768 0.32466 1.20549 1.38 511.98 7.17
F2_26651227-28873440_Ks12.64 -2.14175 2.43056 -1.47325 2.63909 0.87 569.63 -4.91

Notes. The columns denote the source name, proper motion from Libralato et al. (2021) along Galactic longitude l, associated uncertainty, proper motion along Galactic latitude b, associated uncertainty, colour H - KS , and the offset coordinates from Sgr A*. We note the different proper motions of F2_26630347-29161867_Ks12.97 and F2_26650085-28895227_Ks12.15 compared to Table E.1, which may be due to different reference frames.

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