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Table 3.

Integrated magnitudes of Dorado in UVIT FUV.CaF2.

Field ID FUV.CaF2 ϵ ⟨PA⟩ n LFUV.CaF2 SFR
source AB [mag] [deg] 1026 [erg s−1 Hz−1] [M yr−1]
A NGC 1536 15.90 ± 0.02 0.40 160 0.76 ± 0.02 5.95 ± 0.05 0.083 ± 0.001

B NGC 1546 17.24 ± 0.11 0.66 141 0.98 ± 0.04 1.74 ± 0.08 0.024 ± 0.001

C NGC1549 16.92 ± 0.11 0.07 0 2.86 ± 0.28 2.32 ± 0.01 0.033 ± 0.001
[CMI2001]4136-01 19.13 ± 0.34 ... ... ... 0.30 ± 0.04 0.004 ± 0.001

D NGC 1553 16.44 ± 0.13 0.36 150 2.67 ± 0.21 3.63 ± 0.20 0.051 ± 0.003

E IC 2058 16.22 ± 0.04 0.74 18 1.48 ± 0.10 4.43 ± 0.07 0.062 ± 0.001
PGC 075125 18.07 ± 0.10 0.36 20 1.20 ± 0.03 0.81 ± 0.03 0.011 ± 0.0005

F NGC 1566 12.13 ± 0.03 0.05 15 0.94 ± 0.05 175.30 ± 1.93 2.455 ± 0.027

G NGC 1596 17.96 ± 0.21 0.52 20 2.12 ± 0.18 0.95 ± 0.08 0.013 ± 0.001
NGC 1602 15.06 ± 0.04 0.32 80 0.25 ± 0.04 12.94 ± 0.21 0.181 ± 0.003

Notes. Column (2) gives the galaxy identification; Members of Dorado, according to Kourkchi & Tully (2017) are indicated in bold; Col. (3) gives the extinction corrected FUV integrated magnitude; Col. (4) gives the average ellipticity; Col. (5) gives the average PA; Col. (6) gives the Sersíc index; Col. (7) gives the total absolute FUV luminosity; Col. (8) gives the SFR as derived from Eq. (1).

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