Table A.1.
First rows of the proper motion catalogue.
RA | ΔRA | Dec | ΔDec | H | dH | μl | dμl | μb | dμb |
---|---|---|---|---|---|---|---|---|---|
(deg) | (arcsec) | (deg) | (arcsec) | (mag) | (mag) | (mas yr−1) | (mas yr−1) | (mas yr−1) | (mas yr−1) |
266.41925 | 0.00097 | -28.80355 | 0.00068 | 15.21485 | 0.01091 | -4.19960 | 0.94585 | -0.21576 | 0.89140 |
266.38788 | 0.00126 | -28.79402 | 0.00154 | 14.09413 | 0.01906 | 1.51912 | 1.19169 | -0.25583 | 1.44118 |
266.39636 | 0.00139 | -28.78592 | 0.00111 | 16.20390 | 0.01702 | -2.75357 | 1.07579 | 5.50186 | 1.34625 |
266.46149 | 0.00024 | -28.82738 | 0.00028 | 15.90056 | 0.00269 | 3.25698 | 1.23304 | -3.95698 | 0.80972 |
266.45837 | 0.00092 | -28.83129 | 0.00112 | 16.74176 | 0.00426 | -1.01231 | 1.78124 | 0.70804 | 0.72085 |
266.45883 | 0.00035 | -28.81885 | 0.00042 | 12.33349 | 0.00333 | -0.38286 | 0.67396 | -5.06638 | 0.57996 |
266.46439 | 0.00033 | -28.82380 | 0.00042 | 13.23098 | 0.00451 | 0.15466 | 0.63118 | -0.47885 | 0.66669 |
266.46310 | 0.00017 | -28.82315 | 0.00027 | 13.50527 | 0.00324 | 0.81493 | 0.59243 | 1.39099 | 0.55884 |
266.45731 | 0.00042 | -28.81703 | 0.00035 | 13.86630 | 0.00316 | 6.76527 | 0.75450 | 0.18626 | 0.71306 |
266.46158 | 0.00087 | -28.82217 | 0.00100 | 14.26329 | 0.01246 | 1.26582 | 0.63530 | 2.36740 | 0.55892 |
266.45984 | 0.00026 | -28.82113 | 0.00040 | 14.27947 | 0.00237 | 0.73303 | 0.57984 | 0.71113 | 0.56797 |
266.46005 | 0.00046 | -28.82115 | 0.00046 | 14.41241 | 0.00353 | 1.00725 | 0.58351 | -1.34299 | 0.69243 |
266.46002 | 0.00030 | -28.82071 | 0.00031 | 14.60487 | 0.00341 | 1.09343 | 0.58009 | 2.26018 | 0.52826 |
266.46204 | 0.00034 | -28.82129 | 0.00042 | 14.71005 | 0.00485 | -2.38172 | 0.61363 | -0.01849 | 0.56018 |
266.46249 | 0.00035 | -28.82142 | 0.00042 | 14.88699 | 0.00399 | -0.97400 | 0.59609 | 0.30383 | 0.56781 |
266.45737 | 0.00020 | -28.81890 | 0.00020 | 14.89931 | 0.00402 | -5.31594 | 0.66412 | 2.53803 | 0.61431 |
266.46188 | 0.00042 | -28.82163 | 0.00035 | 14.89672 | 0.00324 | -0.38727 | 0.61505 | -0.00836 | 0.77331 |
266.46045 | 0.00042 | -28.82105 | 0.00035 | 15.22904 | 0.00245 | 2.62466 | 0.58435 | 1.66795 | 0.53053 |
266.46039 | 0.00058 | -28.82126 | 0.00050 | 15.43128 | 0.00509 | 0.09456 | 0.58066 | 3.10825 | 0.62786 |
266.46262 | 0.00053 | -28.82263 | 0.00049 | 16.10555 | 0.00687 | 1.81359 | 0.64299 | 4.89179 | 0.56042 |
266.46057 | 0.00061 | -28.82119 | 0.00061 | 16.11472 | 0.00427 | 3.45930 | 0.60339 | 2.09749 | 0.61913 |
266.46198 | 0.00026 | -28.82258 | 0.00023 | 16.15639 | 0.00477 | 1.15596 | 0.58290 | 0.23051 | 0.61128 |
266.45825 | 0.00067 | -28.81790 | 0.00047 | 16.35515 | 0.00604 | -5.25076 | 0.70984 | -1.35620 | 0.67907 |
266.46320 | 0.00056 | -28.82372 | 0.00059 | 16.37724 | 0.00444 | -5.08730 | 0.65269 | -0.07486 | 0.58265 |
266.45694 | 0.00047 | -28.81782 | 0.00067 | 16.44830 | 0.00435 | 5.46795 | 0.76426 | 2.57502 | 0.77120 |
266.46384 | 0.00080 | -28.82331 | 0.00069 | 16.48845 | 0.00920 | -0.67524 | 0.65292 | 1.26968 | 0.60490 |
266.46027 | 0.00096 | -28.82076 | 0.00103 | 16.48476 | 0.03141 | -0.32617 | 0.67995 | 1.69349 | 0.59741 |
266.46173 | 0.00032 | -28.82399 | 0.00031 | 12.03400 | 0.00488 | -0.82098 | 0.50486 | -1.43832 | 0.47763 |
266.45947 | 0.00053 | -28.82145 | 0.00034 | 12.44773 | 0.00979 | 1.21442 | 0.51689 | 0.07001 | 0.46946 |
266.46021 | 0.00033 | -28.82553 | 0.00031 | 12.48363 | 0.00448 | 0.74789 | 0.45218 | -0.35204 | 0.41850 |
266.46112 | 0.00030 | -28.82294 | 0.00022 | 12.56305 | 0.00632 | -1.28993 | 0.50806 | 0.88989 | 0.42835 |
266.45703 | 0.00016 | -28.82382 | 0.00017 | 12.91874 | 0.00407 | -0.64706 | 0.45378 | 0.11141 | 0.40211 |
266.45789 | 0.00040 | -28.82413 | 0.00027 | 13.08759 | 0.00242 | 2.94974 | 0.43846 | -1.99291 | 0.43946 |
… | … | … | … | … | … | … | … | … | … |
Notes. RA, ΔRA and Dec, ΔDec are the right ascension and the declination of the sources (and their corresponding uncertainties). H and dH are the H-band magnitude and its uncertainty. μl, dμl, and μb, dμb are the proper motions in the direction parallel and perpendicular to the Galactic plane (and their corresponding uncertainties).
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