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Table 2.

VLA H I detections.

Field Galaxy ID RA (a) Dec. VHI W20 W50 M(HI) (b) M(HI)/M*(c) g − i(d)
[h m s] [d m s] [km s−1] [km s−1] [km s−1] [108M]
J0204 J0204–1009 02 04 25.6 −10 09 36 1904±3 80±5 65±5 3.04 15.2 0.15
J0204 NGC 811 02 04 34.8 −10 06 30.52 1924±6 175±12 150±12 35.93
J0204 PGC 7892 02 04 12.4 −10 04 42.60 1902±4 95±7 75±7 9.34
J0204 WISEA (e) 02 04 48 −09 59 03 1879±5 75±10 50±10 4.55
J0301 J0301–0052 03 01 49.0 −00 52 57 2193±3 30±6 30±6 0.06 0.2 –0.22
J0315 J0315–0024 03 15 59.9 −00 24 26 6774±2 83±4 78±4 5.99 12.0 –0.07
J0315 KUG 0313–006 03 16 06.10 −00 26 21 6797±10 202±20 176±20 57.91
J0315 UGC 2628 03 16 31.8 −00 28 05 6810±4 404±9 388±9 193.47
J2053 J2053+0039 20 53 12.6 +00 39 14 3944±4 56±8 36±8 0.23 1.2 0.28
J2053 UGC 11645 20 53 24.6 +00 39 07.05 3815±4 306±9 299±9 149.59

Notes.

(a)

All galaxy coordinates are from (Filho et al. 2013) except NGC 811,PGC 7892 and UGC 11645 which are from NED.

(b)

M(HI) = 2.36 × 105D2 ∫Sν dv (Giovanelli & Haynes 1985). D is the distance in Mpc and ∫Sν dv is the integrated flux from our VLA observations, except for UGC 11645 where we use the H I flux (4.49 Jy) from Masters et al. (2014) because the VLA flux for that galaxy was contaminated by RFI.

(c)

Where M* is from Filho et al. (2013).

(d)

SDSS model magnitude colours.

(e)

Full ID, WISEA J020448.18–095859.0.

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