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Table 1.

HI and optical properties of the HI-bearing dwarfs.

ID RA Dec vhelio DHI W50 FHI S/N Mg MB (g − r)0 Survey Morph
[deg] [deg] [km s−1] [Mpc] [km s−1] [Jy-km s−1] mag mag mag
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17)
MATLAS-23 19.7116 3.5617 4933.0 ± 8.0 71.36 ± 0.11 100 1.03 ± 0.08 8.2 9.09 ± 0.06 −15.08 −14.76 0.29 7.88 ± 0.02 18.97 10.33 ALFALFA dI
MATLAS-42 20.6260 8.7614 2422.0 ± 15.0 33.46 ± 0.21 27 0.58 ± 0.05 10.7 8.18 ± 0.06 −15.33 −14.98 0.40 8.14 ± 0.03 1.93 9.00 ALFALFA dI; UDG
MATLAS-121 26.5425 28.8157 3764.0 ± 8.0 52.32 ± 0.11 39 0.50 ± 0.04 8.4 8.51 ± 0.06 −14.29 −13.96 0.36 7.67 ± 0.02 10.42 9.18 ALFALFA dE
MATLAS-122 26.9508 22.1426 2987.0 ± 2.0 40.63 ± 0.03 36 1.40 ± 0.04 21.4 8.74 ± 0.05 −15.18 −14.75 0.62 8.43 ± 0.01 8.45 9.82 ALFALFA dI
MATLAS-124 27.2047 21.5792 3024.0 ± 6.0 42.09 ± 0.09 36 0.60 ± 0.05 8.8 8.40 ± 0.06 −13.76 −13.47 0.21 7.24 ± 0.01 12.67 9.05 ALFALFA dI
MATLAS-125 27.2088 22.1143 3039.0 ± 8.0 42.00 ± 0.12 74 0.13 ± 0.03 6.2 7.70 ± 0.12 −15.72 −15.35 0.47 8.41 ± 0.01 0.45 9.59 ATLAS3D dE,N; TTD
MATLAS-127 27.4368 22.3744 2947.0 ± 8.0 41.76 ± 0.12 90 0.22 ± 0.06 4.8 7.94 ± 0.11 −15.93 −15.57 0.42 8.43 ± 0.00 0.64 9.42 ATLAS3D* dI
MATLAS-132 27.6409 22.0435 2347.0 ± 8.0 34.54 ± 0.12 33 0.05 ± 0.03 3.5 7.17 ± 0.24 −10.95 −10.55 0.57 6.65 ± 0.05 11.12 9.35 ATLAS3D dI
MATLAS-146 29.9250 19.0219 2372.0 ± 8.0 38.47 ± 0.12 58 0.11 ± 0.04 3.6 7.69 ± 0.15 −15.94 −15.57 0.47 8.50 ± 0.00 0.36 9.04 ATLAS3D dE; TTD
MATLAS-154 31.7166 10.9491 1955.0 ± 8.0 28.92 ± 0.12 66 0.12 ± 0.05 3.5 7.41 ± 0.18 −12.96 −12.6 0.42 7.24 ± 0.01 2.86 8.98 ATLAS3D dE

Notes. The columns are as follows: (1) Dwarf ID; (2) Right ascension (J2000); (3) Declination (J2000); (4) Heliocentric velocity; (5) HI distance from Hubble flow; (6) W50 line width; (7) HI flux; (8) Signal-to-noise ratio; (9) log10 of the HI mass; (10) g-band absolute magnitude; (11) B-band absolute magnitude; (12) Galactic extinction corrected g − r color; (13) log10 of the stellar mass; (14) HI-mass-to-light ratio; (15) log10 of the dynamical mass; (16) Survey; (17) Morphology. Based on Poulain et al. (2021) for the dEs, dIs, and nucleated (indicated with “,N”), and on Marleau et al. (2021) for the UDGs. ATLAS3D* means that the dwarf has also been detected in the ALFALFA survey. This table is available in its entirety at the CDS.

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