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Table B.1.

AGB stars in the Leo A galaxy.

ID RA(J2000) Dec(J2000) B V I R Hα eB eV eI eR eHα J H Ks DPR Flag (a)
(deg) (deg) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (M⊙ yr−1)
AGB01 149.7874 30.7744 23.575 22.006 20.222 21.099 21.121 0.007 0.009 0.008 0.004 0.010 – – – – 0
AGB02 149.8133 30.7679 23.251 21.476 19.857 20.590 20.612 0.013 0.006 0.006 0.006 0.006 – – – – 0
AGB03 149.8155 30.7269 23.894 21.994 20.174 20.942 20.972 0.009 0.012 0.006 0.007 0.007 – – – – 0
AGB04 149.8168 30.7715 22.991 21.279 19.668 20.321 20.329 0.011 0.011 0.008 0.006 0.006 – – – – 0
AGB05 149.8195 30.7319 23.788 22.020 20.308 20.976 20.996 0.012 0.011 0.005 0.008 0.004 – – – – 0
AGB06 149.8200 30.7485 24.119 21.990 19.490 20.670 20.790 0.024 0.009 0.004 0.005 0.004 – – – – 1
AGB07 149.8240 30.7483 23.193 21.761 20.184 20.922 20.910 0.010 0.024 0.004 0.017 0.009 – – – – 0
AGB08 149.8255 30.7379 24.977 22.380 19.595 20.704 20.805 0.022 0.014 0.004 0.004 0.005 – – – – 1
AGB09 149.8285 30.7396 23.750 21.946 20.166 20.738 20.745 0.032 0.016 0.006 0.004 0.005 – – – – 0
AGB10 149.8288 30.7480 22.782 21.017 19.252 20.183 20.212 0.019 0.009 0.010 0.004 0.009 – – – – 0
AGB11 149.8331 30.7473 23.504 21.638 19.627 20.729 20.757 0.073 0.051 0.010 0.007 0.011 17.71 16.76 – 4.2E−11 0
AGB12 149.8364 30.7608 24.256 22.138 19.709 20.680 20.794 0.038 0.008 0.006 0.007 0.007 18.23 17.13 16.25 6.4E−12 1
AGB13 149.8377 30.7437 24.170 21.971 19.871 20.802 20.818 0.053 0.018 0.007 0.005 0.005 18.23 17.58 16.66 2.8E−12 0
AGB14 149.8440 30.7405 24.478 22.281 19.646 20.771 20.873 0.070 0.019 0.009 0.007 0.005 17.56 16.80 15.99 1.0E−10 1
AGB15 149.8460 30.7614 25.094 22.309 19.630 20.597 20.694 0.047 0.016 0.004 0.004 0.007 17.61 16.94 15.80 6.1E−11 1
AGB16 149.8551 30.7566 23.096 21.307 19.392 20.051 20.080 0.024 0.010 0.006 0.005 0.004 17.64 17.05 16.31 4.0E−12 0
AGB17 149.8554 30.7310 22.953 21.508 19.923 20.596 20.593 0.013 0.010 0.004 0.005 0.007 18.24 17.76 – 4.5E−13 0
AGB18 149.8572 30.7359 24.149 22.202 20.174 21.138 21.202 0.061 0.020 0.004 0.004 0.008 18.41 17.77 – – 0
AGB19 149.8589 30.7476 24.306 22.401 19.621 20.808 20.918 0.126 0.021 0.004 0.005 0.006 17.81 16.86 15.86 2.1E−10 1
AGB20 149.8596 30.7310 23.267 21.558 19.812 20.676 20.693 0.019 0.014 0.009 0.005 0.004 17.58 – 16.59 – 0
AGB21 149.8619 30.7527 24.264 22.169 20.089 21.188 21.253 0.064 0.027 0.004 0.007 0.010 18.44 17.95 16.78 2.1E−12 0
AGB22 149.8696 30.7300 23.139 21.522 19.911 20.679 20.687 0.016 0.004 0.004 0.004 0.008 18.45 17.88 – 4.0E−13 0
AGB23 149.8731 30.7621 22.633 21.198 19.702 20.389 20.377 0.028 0.018 0.007 0.006 0.006 18.14 17.67 16.79 5.9E−13 0
AGB24 149.8732 30.7479 23.208 21.686 20.155 20.913 20.921 0.012 0.010 0.004 0.006 0.007 18.62 18.11 – 3.2E−13 0
AGB25 149.8744 30.7578 23.385 21.619 19.951 20.709 20.730 0.012 0.008 0.005 0.005 0.009 18.41 17.77 – 2.4E−12 0
AGB26 149.8915 30.7274 22.966 21.388 19.791 20.524 20.528 0.010 0.006 0.006 0.004 0.004 – 17.76 16.83 – 0
AGB27 149.8928 30.7286 25.329 22.829 20.064 19.989 20.015 0.045 0.025 0.007 0.004 0.004 17.02 16.00 15.08 1.3E−09 1
AGB28 149.8937 30.7456 23.572 21.765 20.303 21.003 21.009 0.230 0.026 0.006 0.012 0.004 19.07 18.37 – 3.3E−13 0
AGB29 149.8965 30.7431 24.908 22.508 19.991 21.343 21.436 0.040 0.024 0.004 0.008 0.009 17.97 17.37 16.31 6.0E−12 1
AGB30 149.8974 30.7473 23.462 21.613 19.784 20.509 20.528 0.014 0.010 0.006 0.005 0.006 18.39 17.40 – 3.0E−12 0
AGB31 149.8977 30.7072 23.054 21.516 19.932 20.659 20.655 0.010 0.008 0.004 0.006 0.004 – – – – 0
AGB32 149.9815 30.6830 24.246 21.654 19.290 20.256 20.324 0.027 0.005 0.006 0.004 0.004 – – – – 1
cAGB01 149.8450 30.7320 23.718 22.209 20.098 21.195 21.097 0.021 0.004 0.005 0.006 0.011 18.50 18.25 – 1.8E−12 0
cAGB02 149.8633 30.7440 24.769 23.379 20.644 23.090 23.045 0.008 0.067 0.007 0.087 0.113 17.58 16.79 15.59 1.2E−09 1
cAGB03 149.8891 30.7372 25.286 23.411 20.166 22.332 22.122 0.033 0.028 0.006 0.018 0.014 18.02 17.74 16.91 4.5E−12 1

Notes. JHKs magnitudes and dust production rates (DPRs) are from Jones et al. (2018).

(a)

0: no dust. 1: possible circumstellar dusty envelopes based on the colour (V − I > 2.3) of the AGB stars in the CMD.

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