ID R.A.
(J2000)
Decl.
(J2000)
mRa
(mag)
B-Rb
(mag)
μ0,Rc
(mag arcsec-2)
nc
rec
(arcsec)
MRd
(mag)
log Me
(Msun)
DW
N1291-DW1
(profile)
3:19:25.9 -40:03:47 17.46 ± 0.13 1.31 24.18 ± 0.19 0.65 ± 0.03 11.30 ± 0.23 -12.34 6.97
DW
N1291-DW2
(profile)
3:15:09.7 -40:40:05 17.05 ± 0.13 1.17 24.61 ± 0.19 0.65 ± 0.03 16.62 ± 0.38 -12.75 7.03
DW
N1291-DW3
(profile)
3:17:29.4 -40:58:22 16.25 ± 0.05 1.36 23.81 ± 0.07 0.71 ± 0.01 17.30 ± 0.17 -13.55 7.45
DW
N1291-DW4
(profile)
3:19:43.1 -41:26:54 16.44 ± 0.08 1.28 24.25 ± 0.13 0.60 ± 0.02 18.47 ± 0.26 -13.36 7.42
DW
N1291-DW5
(profile)
3:17:38.1 -41:41:45 16.76 ± 0.10 1.16 24.57 ± 0.14 0.77 ± 0.02 20.32 ± 0.42 -13.04 7.15
DW
N1291-DW6f
(profile)
3:18:43.0 -41:01:27 17.44 ± 0.18 1.14 23.09 ± 0.24 0.88 ± 0.04 8.24 ± 0.17 -12.36 6.87
DW
N1291-DW7f
(profile)
3:21:24.4 -41:59:44 15.50 ± 0.04 1.13 23.34 ± 0.06 0.58 ± 0.01 17.86 ± 0.14 -14.30 7.48
DW
N1291-DW8f
(profile)
3:17:01.4 -41:42:01 15.75 ± 0.10 1.23 22.95 ± 0.13 0.82 ± 0.02 15.88 ± 0.24 -14.05 7.59
DW
N1291-DW9
(profile)
3:09:25.1 -41:04:57 18.42 ± 0.18 1.20 23.90 ± 0.23 0.84 ± 0.04 7.37 ± 0.14 -11.38 6.47
DW
N1291-DW10
(profile)
3:25:38.4 -41:13:51 17.16 ± 0.23 1.11 25.08 ± 0.32 0.72 ± 0.05 20.60 ± 0.82 -12.64 6.99
DW
N1291-DW11
(profile)
3:12:44.2 -42:47:54 17.51 ± 0.32 0.81 23.99 ± 0.44 0.80 ± 0.07 11.63 ± 0.54 -12.36 6.59
DW
N1291-DW12
(profile)
3:18:47.0 -42:11:58 19.81 ± 0.36 1.12 25.19 ± 0.54 0.75 ± 0.09 7.22 ± 0.26 -9.99 5.98
DW
N1291-DW13
(profile)
3:20:33.8 -40:48:18 17.81 ± 0.34 1.22 26.39 ± 0.55 0.48 ± 0.08 23.60 ± 1.89 -11.99 6.62
DW
N1291-DW14f
(profile)
3:25:02.8 -40:21:32 17.94 ± 0.48 1.02 22.66 ± 0.63 0.80 ± 0.11 4.56 ± 0.18 -11.86 6.45
DW
N1291-DW15
(profile)
3:19:37.7 -40:25:17 18.65 ± 0.32 1.07 22.83 ± 0.38 1.07 ± 0.22 4.82 ± 0.22 -11.15 6.20

Notes. Magnitudes and surface brightnesses are uncorrected for Galactic extinction.
a Apparent magnitude calculated by Equation Ltot = 2πI0rs2nΓ(2n), where I0 is the intensity at the center, rs is the scale length, and Γ is the gamma function.
b Color measured within twice the effective radius derived from R-band image.
c Central surface brightness (μ0,R), Sersic index (n), and effective radius (re) in the R-band image derived from the 1-D profile fit.
d Absolute magnitude calculated by assuming that the dwarfs are at the same distance as NGC 1291 (d = 9.08 Mpc).
e Stellar mass estimated with an equation of log M/L = 0.872×(B-R)-0.866 adopted from Into & Portinari (2013).
f Cross-ID: [MDS99] F301-056, [MDS99] F301-044, [MDS99] F301-064, LEDA 587327, respectively.