Table B.1.
Example page of our dwarf galaxy catalog that includes likely cluster galaxies.
Target | R.A. | Dec. | b/a | θ | mr′ | Re | n | u’ | g’ | r’ | i’ | C | RFF | Morphology |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
FDSLSB1 | 55.6888 | -35.4720 | 0.80 ± 0.06 | 10.6 ± 3.6 | 21.7 ± 0.2 | 2.0 ± 0.4 | 0.3 ± 0.4 | 23.43 ± 0.15 | 22.96 ± 0.13 | 22.78 ± 0.11 | 22.35 ± 0.07 | 1.9 | -0.00 | 2 |
FDSLSB2 | 55.3600 | -35.3797 | 0.84 ± 0.06 | 52.5 ± 3.8 | 21.2 ± 0.3 | 2.7 ± 0.6 | 0.5 ± 0.4 | 24.52 ± 0.71 | 22.51 ± 0.14 | 21.90 ± 0.09 | 21.63 ± 0.07 | 2.9 | -0.02 | 1 |
FDSLSB3 | 56.0367 | -35.1445 | 0.83 ± 0.03 | 32.8 ± 2.3 | 20.6 ± 0.2 | 2.0 ± 0.3 | 0.9 ± 0.3 | 23.62 ± 0.17 | 22.34 ± 0.08 | 21.69 ± 0.06 | 21.40 ± 0.05 | 2.7 | -0.00 | 1 |
FDSLSB4 | 55.5467 | -35.4432 | 0.62 ± 0.09 | 61.5 ± 5.0 | 18.8 ± 0.3 | 11.2 ± 3.1 | 0.8 ± 0.4 | 21.43 ± 0.51 | 20.25 ± 0.18 | 19.72 ± 0.12 | 19.35 ± 0.09 | 2.2 | 0.00 | 1 |
FDSLSB5 | 55.6311 | -35.0248 | 0.92 ± 0.09 | 24.7 ± 4.8 | 21.3 ± 0.3 | 3.3 ± 0.9 | 0.8 ± 0.4 | 23.78 ± 0.58 | 22.78 ± 0.27 | 22.19 ± 0.16 | 22.07 ± 0.13 | 2.5 | -0.05 | 1 |
FDSLSB6 | 55.3456 | -35.8966 | 0.40 ± 0.11 | 10.7 ± 6.1 | 20.8 ± 0.3 | 5.5 ± 1.7 | 1.4 ± 0.4 | 23.62 ± 0.60 | 22.28 ± 0.20 | 21.73 ± 0.13 | 21.81 ± 0.12 | 2.6 | 0.01 | 1 |
FDSLSB7 | 55.6970 | -35.3898 | 0.66 ± 0.10 | -39.7 ± 5.5 | 21.8 ± 0.3 | 3.1 ± 0.9 | 0.3 ± 0.4 | 24.27 ± 0.59 | 23.21 ± 0.26 | 22.68 ± 0.17 | 22.49 ± 0.12 | 2.4 | 0.00 | 1 |
FDSLSB8 | 56.2119 | -35.7884 | 0.43 ± 0.14 | 88.4 ± 7.0 | 21.2 ± 0.4 | 5.4 ± 1.9 | 1.6 ± 0.4 | 23.91 ± 0.79 | 22.83 ± 0.33 | 22.40 ± 0.23 | 21.57 ± 0.10 | 2.9 | -0.04 | 1 |
FDSLSB9 | 56.3158 | -35.2712 | 0.56 ± 0.06 | 9.5 ± 3.3 | 21.2 ± 0.2 | 2.4 ± 0.5 | 1.1 ± 0.4 | 23.68 ± 0.18 | 22.74 ± 0.11 | 22.25 ± 0.08 | 22.29 ± 0.06 | 2.6 | -0.02 | 2 |
FDSLSB10 | 55.7587 | -35.3283 | 0.48 ± 0.14 | -1.0 ± 7.3 | 20.7 ± 0.4 | 7.3 ± 2.6 | 0.4 ± 0.4 | 23.79 ± 1.46 | 21.90 ± 0.28 | 21.49 ± 0.20 | 21.04 ± 0.12 | 2.0 | -0.01 | 2 |
FDSLSB11 | 55.8614 | -35.4978 | 0.74 ± 0.06 | 18.5 ± 3.3 | 21.8 ± 0.2 | 1.8 ± 0.4 | 0.7 ± 0.4 | 24.19 ± 0.21 | 23.48 ± 0.15 | 22.90 ± 0.10 | 22.22 ± 0.05 | 2.7 | -0.00 | 1 |
FDSLSB12 | 55.2824 | -35.4126 | 0.71 ± 0.04 | 8.7 ± 2.6 | 20.6 ± 0.2 | 2.3 ± 0.4 | 0.9 ± 0.3 | 22.91 ± 0.11 | 21.83 ± 0.07 | 21.59 ± 0.06 | 21.38 ± 0.05 | 2.8 | -0.00 | 1 |
FDSLSB13 | 55.3112 | -35.4510 | 0.76 ± 0.05 | -51.1 ± 3.3 | 19.9 ± 0.2 | 4.1 ± 0.9 | 0.8 ± 0.4 | 22.10 ± 0.17 | 20.97 ± 0.08 | 20.58 ± 0.06 | 20.29 ± 0.05 | 2.4 | 0.00 | 4 |
FDSLSB14 | 56.1882 | -35.2697 | 0.76 ± 0.13 | -20.2 ± 6.8 | 20.4 ± 0.4 | 7.6 ± 2.6 | 0.3 ± 0.4 | 22.89 ± 1.09 | 21.80 ± 0.42 | 21.14 ± 0.23 | 21.08 ± 0.21 | 1.6 | -0.02 | 1 |
FDSLSB15 | 55.9851 | -35.8301 | 0.71 ± 0.08 | -25.3 ± 4.7 | 21.0 ± 0.3 | 3.7 ± 1.0 | 1.0 ± 0.4 | 24.15 ± 0.77 | 22.50 ± 0.20 | 21.95 ± 0.13 | 22.08 ± 0.12 | 2.7 | -0.01 | 1 |
FDSLSB16 | 56.2082 | -35.5355 | 0.96 ± 0.06 | -39.0 ± 3.6 | 21.2 ± 0.2 | 2.5 ± 0.6 | 0.4 ± 0.4 | 24.86 ± 0.92 | 22.67 ± 0.16 | 22.16 ± 0.11 | 22.15 ± 0.09 | 2.2 | 0.01 | 1 |
FDSLSB17 | 56.1431 | -35.1818 | 0.78 ± 0.02 | -38.2 ± 1.4 | 15.4 ± 0.1 | 11.9 ± 1.5 | 1.7 ± 0.3 | 18.35 ± 0.06 | 16.82 ± 0.03 | 16.20 ± 0.03 | 15.90 ± 0.04 | 3.3 | 0.01 | 1 |
FDSLSB18 | 55.8573 | -35.2292 | 0.35 ± 0.13 | -1.6 ± 6.9 | 21.2 ± 0.4 | 5.4 ± 1.8 | 0.6 ± 0.4 | 24.13 ± 0.79 | 22.62 ± 0.23 | 22.03 ± 0.14 | 21.46 ± 0.08 | 2.4 | 0.03 | 1 |
FDSLSB19 | 49.9763 | -36.4139 | 0.92 ± 0.03 | 39.4 ± 2.1 | 20.1 ± 0.2 | 2.2 ± 0.4 | 0.9 ± 0.3 | -1.00 ± -1.00 | 21.39 ± 0.06 | 21.00 ± 0.05 | 20.83 ± 0.04 | 2.9 | 0.02 | 1 |
FDSLSB20 | 49.8691 | -36.8686 | 0.82 ± 0.04 | -32.3 ± 2.8 | 21.0 ± 0.2 | 2.0 ± 0.4 | 1.0 ± 0.3 | -1.00 ± -1.00 | 22.51 ± 0.10 | 22.01 ± 0.07 | 21.70 ± 0.05 | 2.7 | 0.01 | 1 |
... |
Notes. The columns from left to right correspond to: target, right ascension (R.A.) and declination (Dec.) in ICRS coordinates, axis ratio (b/a), position angle measured from north to east (θ), apparent r’-band total magnitude (mr′), r’-band effective radius in arcseconds (Re), Sérsic index (n), aperture magnitudes within the effective radius in the u’, g’, r’, and i’ filters, the concentration index (C), and the residual flux fraction (RFF). The values after the ±-signs correspond to the 1σ uncertainties in the parameters. The last column tells the tidal morphological type of the galaxy according to our classifications in Sect. 5: “1” corresponds to a regular galaxy, “2” to a slightly disturbed galaxy, “3” to a clearly disturbed galaxy, and “4” to an unclear case, and asterisk at the end of the morphological classification indicates that the object has a nucleus.
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