Table 2.
Global properties of the sample.
Apertif name | Literature name | D | Vsys | W50 | FH I | log | log | log | |
---|---|---|---|---|---|---|---|---|---|
AHC- | [Mpc] | [km s−1] | [km s−1] | [Jy km s−1] | (MH I/M⊙) | (M⋆/M⊙) | (Mb/M⊙) | ||
1 | J020345.3+371444 | − | 50 | 4526 ± 4 | 36 | 0.99 | ![]() |
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2 | J020345.3+371444 | a ( * ) | 50 | 4517 ± 4 | 36 | 3.39 | ![]() |
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3 | J133650.2+320534 | UGC 8605 | 48 | 3004 ± 4 | 55 | 2.46 | ![]() |
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4 | J133650.2+320534 | UGC 8602 | 48 | 3066 ± 4 | 77 | 1.78 | ![]() |
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5 | J101017.8+582856 | CGCG 290-011 | 35 | 2134 ± 4 | 70 | 1.25 | ![]() |
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6 | J101017.8+582856 | UGC 5480 | 35 | 2158 ± 4 | 110 | 3.53 | ![]() |
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7 | J133045.2+324548 | UGC 8503 | 67 | 4680 ± 4 | 56 | 3.81 | ![]() |
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8 | J133042.2+294735 | AGC 239039 | 47 | 2949 ± 4 | 86 | 2.02 | ![]() |
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9 | J133507.0+313118 | AGC 234932 | 70 | 4953 ± 4 | 49 | 1.38 | ![]() |
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10 | J133704.8+315336 | AGC 239112 | 48 | 3022 ± 4 | 48 | 1.28 | ![]() |
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11 | J101655.0+582325 | UGC 5541 | 37 | 2265 ± 4 | 139 | 5.57 | ![]() |
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12 | J130830.2+543756 | b ( * ) | 42 | 2542 ± 4 | 95 | 6.94 | ![]() |
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13 | J135938.5+372631 | c ( * ) | 42 | 2710 ± 4 | 51 | 2.95 | ![]() |
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14 | J220741.6+400853 | − | 56 | 4702 ± 4 | 129 | 3.00 | ![]() |
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15 | J220743.8+414343 | d ( * ) | 78 | 5705 ± 4 | 135 | 2.62 | ![]() |
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16 | J223258.7+393853 | − | 47 | 3999 ± 5 | 132 | 2.17 | ![]() |
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17 | J223902.0+383211 | − | 53 | 4546 ± 5 | 59 | 1.98 | ![]() |
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18 | J221640.4+402424 | − | 55 | 4612 ± 4 | 78 | 1.14 | ![]() |
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19 | J221800.3+405946 | − | 50 | 4262 ± 4 | 139 | 1.61 | ![]() |
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20 | J222407.1+411511 | UGC 12027 | 48 | 4133 ± 4 | 93 | 4.80 | ![]() |
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21 | J131846.6+274359 | UGC 8363 | 38 | 2455 ± 5 | 144 | 7.79 | ![]() |
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22 | J133339.8+602315 | UGCA 363 | 32 | 2066 ± 5 | 34 | 5.14 | ![]() |
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23 | J222230.6+360028 | UGC 12005 | 73 | 5476 ± 4 | 54 | 3.93 | ![]() |
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24 | J224941.0+394852 | − | 69 | 5349 ± 4 | 35 | 4.66 | ![]() |
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Notes. The first six galaxies are galaxies found in pairs. D is distance with errors of 15%. Vsys is systemic velocity given in the optical convention and the barycentric rest frame. W50 is the width of the global profile at 50% peak emission, with errors of the same order as Vsys. FH I is the total H I flux of the source with errors of 15%. MH I, M⋆, and Mb are H I, stellar, and baryonic masses, respectively.
( * )(a) WISEA J020343.19+371442.6, (b) SDSS J130830.62+543757.4, (c) WISEA J135937.97+372636.1, (d) UGC 11919:[SJZ2013] 22.
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