Table 3
Sample of new LSBGs identified in this work.
COADD_ID | RA (deg) | Dec (deg) | ggf | gcor | ![]() |
rg1/2 (arcsec) | n | q | log10(Σstar) (M⊙ kpc−2) | ![]() |
igf | icor | ![]() |
ri,1/2 (arcsec) | ![]() |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
61 456 395 | 29.7062 | −60.4882 | 19.06 | 18.97 | 25.41 | 9.41 | 2.17 | 0.62 | 5.86 | 1.06 | 18.72 | 18.67 | 25.37 | 10.86 | 1.03 |
61 508 029 | 29.925 | 4.60483 | 19.84 | 19.67 | 24.33 | 3.43 | 0.72 | 0.85 | 6.82 | 1.03 | 19.27 | 19.19 | 23.52 | 3.06 | 0.99 |
61 580 602 | 30.3125 | −58.1927 | 18.89 | 18.83 | 24.56 | 5.99 | 1.5 | 0.82 | 6.87 | 1.02 | 18.07 | 18.04 | 23.72 | 5.93 | 1.02 |
61 638 403 | 29.9539 | 4.75811 | 20.02 | 19.87 | 24.28 | 3.84 | 0.74 | 0.54 | 6.52 | 1.04 | 19.61 | 19.53 | 23.62 | 3.45 | 1 |
61 638 933 | 29.4862 | 4.74468 | 19.2 | 19.06 | 24.24 | 4.59 | 0.93 | 0.79 | 6.82 | 0.98 | 18.7 | 18.63 | 23.38 | 3.89 | 0.99 |
61 712 539 | 30.2824 | 5.28992 | 19.67 | 19.53 | 24.26 | 4.57 | 1.01 | 0.52 | 6.58 | 1.01 | 19.47 | 19.4 | 23.2 | 3.07 | 1.03 |
61 766 250 | 30.1112 | −9.24769 | 20.76 | 20.69 | 26.29 | 7.8 | 1.47 | 0.42 | 5.87 | 1.13 | 20.19 | 20.15 | 25.2 | 6.15 | 1.1 |
6 2011 325 | 29.9449 | −6.78979 | 21.6 | 21.51 | 25.91 | 3.17 | 0.5 | 0.84 | 6.27 | 1.02 | 20.8 | 20.76 | 25.21 | 3.31 | 1 |
6 2053 525 | 29.8595 | −16.8586 | 19.87 | 19.8 | 24.24 | 3.49 | 0.87 | 0.73 | 6.81 | 1.03 | 19.32 | 19.29 | 23.41 | 3.06 | 1.02 |
6 2071 354 | 29.8342 | −17.1604 | 20.53 | 20.46 | 24.47 | 3.01 | 0.84 | 0.66 | 6.71 | 0.99 | 19.91 | 19.87 | 23.65 | 2.75 | 0.99 |
6 222 7622 | 29.5063 | −13.3511 | 20.84 | 20.79 | 24.88 | 2.68 | 0.68 | 0.91 | 7.24 | 1.02 | 19.97 | 19.94 | 22.96 | 1.66 | 1.05 |
6 2371 677 | 29.6675 | −5.35506 | 19.7 | 19.62 | 24.25 | 3.54 | 0.79 | 0.84 | 6.97 | 1.05 | 19 | 18.96 | 23.32 | 3.2 | 1.03 |
62 646 182 | 30.4643 | −24.0018 | 18.46 | 18.4 | 24.44 | 6.88 | 1.19 | 0.83 | 6.77 | 1 | 17.98 | 17.95 | 23.59 | 5.8 | 0.97 |
6 2830 903 | 29.9594 | −28.8656 | 20.11 | 20.07 | 24.35 | 2.94 | 0.71 | 0.91 | 7.56 | 1.03 | 19.01 | 18.99 | 22.44 | 2.03 | 1.04 |
62 840 965 | 30.1905 | −6.18018 | 20.18 | 20.1 | 24.35 | 2.74 | 0.76 | 0.98 | 7.35 | 1.01 | 19.22 | 19.18 | 22.85 | 2.14 | 1 |
63 037 584 | 28.9741 | −59.5261 | 19.46 | 19.39 | 24.4 | 6.33 | 0.9 | 0.38 | 6.31 | 1.01 | 18.88 | 18.85 | 23.99 | 6.81 | 1.01 |
63 097 874 | 29.3755 | −61.1452 | 20.6 | 20.51 | 24.87 | 3.08 | 1.02 | 0.85 | 6.58 | 1.02 | 20.29 | 20.25 | 23.86 | 2.23 | 1.02 |
63 113 174 | 29.1535 | −61.4326 | 18.81 | 18.72 | 24.78 | 6.73 | 0.8 | 0.86 | 6.47 | 1 | 18.52 | 18.47 | 24.15 | 5.76 | 0.99 |
63 262 376 | 30.2929 | −24.9787 | 21.48 | 21.43 | 26.1 | 3.92 | 0.98 | 0.73 | 6.18 | 1.03 | 20.62 | 20.6 | 25.35 | 4.12 | 1.04 |
63 527 438 | 30.1134 | −4.56234 | 18.8 | 18.73 | 24.51 | 6.72 | 0.42 | 0.68 | 6.2 | 1.02 | 18.68 | 18.65 | 24.37 | 6.63 | 0.99 |
63 716 543 | 30.0657 | −39.5446 | 20.58 | 20.52 | 25.1 | 3.73 | 1.16 | 0.74 | 6.67 | 1.02 | 19.84 | 19.81 | 24.01 | 3.17 | 1.01 |
63 922 768 | 29.5244 | −32.7958 | 18.41 | 18.35 | 24.6 | 7.62 | 1.61 | 0.83 | 6.59 | 1.08 | 18.06 | 18.03 | 23.87 | 6.37 | 1.04 |
64 480 503 | 29.4619 | −23.0107 | 18.98 | 18.94 | 24.33 | 5.05 | 0.91 | 0.86 | 6.81 | 1.04 | 18.5 | 18.48 | 23.54 | 4.39 | 1 |
64 560 481 | 30.0521 | −5.09785 | 18.18 | 18.1 | 24.36 | 7.21 | 1.17 | 0.91 | 6.86 | 1.06 | 17.66 | 17.62 | 23.49 | 6.14 | 1.01 |
64 697 654 | 29.5818 | −8.50243 | 18.36 | 18.28 | 24.25 | 6.46 | 1 | 0.87 | 6.81 | 0.97 | 17.87 | 17.83 | 23.53 | 5.78 | 0.96 |
64 773 733 | 29.0012 | −50.2462 | 19.39 | 19.32 | 24.7 | 5.13 | 1.4 | 0.8 | 6.66 | 1.03 | 18.94 | 18.91 | 23.78 | 4.13 | 1.01 |
64 868 340 | 29.3394 | −23.8729 | 19.43 | 19.38 | 24.2 | 3.72 | 0.86 | 0.93 | 7.63 | 1.02 | 18.36 | 18.34 | 22.23 | 2.47 | 1.26 |
Notes. ‘COADD_ID’ is the unique id of the source, and ‘RA’ and ‘Dec’ gives the sky coordinates of the source as estimated from DES Y3 Gold catalogue (Sevilla-Noarbe et al. 2021). Columns ‘ggf’, ‘gcor’, ‘’, and ‘rg1/2’ represent the magnitude in g band, the g band magnitude after correcting for Galactic extinction, mean surface brightness, and the half-light radius for the g-band fitting using Galfit, respectively. The columns ‘n’, ‘q’, and log10(Σstar) represent the Sérsic index, axis ratio, and the stellar mass density, respectively. Column; ‘
’ represents the reduced chi-square value for the g-band fitting using Galfit. Similarly, columns ‘igf’, icor’, ‘
’,‘ri1/2’, and ‘
’ represent the magnitude in i band, the i band magnitude after correcting for Galactic extinction, the mean surface brightness, the half-light radius, and the reduced chi-square value for the i band fitted using Galfit, respectively.
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