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Table 4

Derived quantities for the early-type galaxies detected with HeViCS.

VCC Type MB Dist. Mdust Tdust Mstar Bands MHI MH2 Ref. (H2)c
GM Mpc 104 M⊙ K 108 M⊙ for Mstar 107 M⊙ 107 M⊙
94 2 –19.04 32.0 325 ± 83 19.1 ± 1.5 133 ± 40 BVH 180.2 <9 Y11
150 –1 –11.30 17.0 13.5 ± 6.7 15.6a 0.049 ± 0.013 gi <3.6
165 1 –16.42 17.0 72 ± 13 16.7 ± 0.7 9.9 ± 4.4 BH <7.9
209 –3 –16.14 17.0 87 ± 13 17.9 ± 0.6 3.4 ± 0.9 giH 3.9
218 –3 –16.41 17.0 20.1 ± 4.0 17.6a 2.7 ± 1.8 BH <3.6
220 1 –19.66 32.0 176 ± 30 19.4 ± 0.8 334 ± 98 BVH <27.9 <8 Y11
270 2 –17.59 32.0 76 ± 16 22.8 ± 1.2 25 ± 13 BH <27.9
278 –3 –16.81 23.0 31 ± 7 17.6a 10 ± 5 BH <6.6
292 –1 –15.60 32.0 49 ± 37 14.7 ± 2.3 2.3 ± 0.6 gi <12.9
312 1 –19.00 32.0 83 ± 33 17.6 ± 1.5 206 ± 92 BH <27.9 <6 Y11
327 1 –17.81 32.0 142 ± 35 17.7 ± 0.9 7.0 ± 4.7 BH <27.9
345 0 –21.29 32.0 64 ± 5b 21.3a 2079 ± 198 BVH <27.9 <5 C07
408 1 –20.34 32.0 314 ± 37 23.8 ± 0.9 690 ± 204 BVH <27.9 <8 Y11
411 1 –17.35 23.0 98 ± 16 19.7 ± 0.8 35 ± 16 BH <14.4
450 1 –16.82 23.0 82 ± 14 20.9 ± 0.9 4.6 ± 2.8 BH 4.6
462 2 –17.74 17.0 95 ± 11 21.9 ± 0.8 49 ± 15 BVH <7.9 4.6 ± 0.4 Y11
482 2 –16.46 17.0 32 ± 22 14.6 ± 2.0 13 ± 4 BVH <7.9
486 2 –17.39 23.0 9.0 ± 7.6 21.6 ± 3.8 28 ± 10 BVH <14.4
498 –1 –12.76 17.0 20.8 ± 6.8 15.6a 0.13 ± 0.04 gi <3.6
571 1 –17.16 23.0 110 ± 27 16.1 ± 0.9 6.5 ± 4.1 BH <14.4
622 –1 –15.20 23.0 30.4 ± 11.1 15.6a 0.29 ± 0.08 gi <6.6
672 1 –17.69 23.0 60 ± 12 20.5 ± 1.0 20 ± 8 BVH <14.4
685 1 –19.28 17.0 25.8 ± 4.5 30.9 ± 2.1 237 ± 77 BVH e <1.5 Y11
705 –1 –14.04 17.0 30 ± 19 15.0 ± 2.0 0.55 ± 0.15 gi <3.6
710 –3 –16.41 17.0 64 ± 14 16.4 ± 0.8 1.4 ± 0.7 BVH 7.8
758 1 –18.22 23.0 611 ± 61 22.1 ± 0.7 101 ± 30 BVH 8.7
763 0 –21.07 17.0 20.0 ± 2.7b 29.0 ± 1.0 1309 ± 182 BVH <7.9 <1.7 Y11
764 1 –16.33 17.0 30.4 ± 8.7 18.6 ± 1.1 4.9 ± 1.4 giH 6.8
781 –3 –16.60 17.0 28.4 ± 9.4 18.4 ± 1.3 5.6 ± 2.3 BVH <3.6
788 –1 –15.49 17.0 17.5 ± 7.2 15.6a 1.3 ± 0.8 BH <3.6
832 –1 –12.30 17.0 19 ± 12 16.4 ± 2.1 0.26 ± 0.06 gi <3.6
881C 0 –21.22 17.0 29.7 ± 7.2 21.0 ± 1.2 1646 ± 422 BVH 8.9
881SE 249 ± 56 13.9 ± 0.7 2.0 ± 0.2 D12
951 –2 –16.91 17.0 27.4 ± 6.8 20.0 ± 1.1 7.2 ± 2.7 BVH <3.6
1003 2 –20.14 17.0 228 ± 23 25.3 ± 0.9 682 ± 178 BVH <7.9 11.2 ± 0.8 Y11
1030 1 –19.44 17.0 266 ± 28 23.9 ± 0.9 250 ± 83 BVH <7.9 7.4 ± 0.7 Y11
1154 1 –19.98 17.0 189 ± 20 25.8 ± 1.0 413 ± 104 BVH <7.9 17.4 ± 0.8 C07
1175 0 –15.92 23.0 7.1 ± 1.9 21.3a 1.8 ± 1.2 BH <14.4
1226 0 –21.94 17.0 31 ± 5 21.3a 2444 ± 658 BVH <7.9 <1.8 Y11
1250 1 –18.37 17.0 120 ± 14 23.0 ± 0.9 45 ± 15 BVH d 11 ± 1 Y02
1253 2 –19.98 17.0 57 ± 8 25.3 ± 1.1 353 ± 104 BVH <7.9 3.5 ± 0.5 C07
1316 0 –21.67 17.0 21.9 ± 1.8b 21.3a 1725 ± 197 BVH d <1.5 C07
1327 0 –17.99 17.0 8.4 ± 1.5 21.3a 113 ± 22 BVH d
1420 –1 –14.87 17.0 50 ± 15 16.3 ± 1.2 1.2 ± 0.3 BVH d
1512 –3 –15.65 17.0 19.5 ± 4.9 17.6a 2.0 ± 1.2 BH <3.6
1535 1 –20.64 17.0 1096 ± 106 23.7 ± 0.8 877 ± 259 BVH 1.4 39 ± 1 C07
1578 –1 –11.57 17.0 27.4 ± 8.5 15.6a 0.015 ± 0.004 gi <3.6
1614 1 –16.91 17.0 8.6 ± 2.7 21.2a 8.8 ± 5.0 BH <7.9
1619 0 –18.82 17.0 25.5 ± 5.1 21.7 ± 1.0 106 ± 32 BVH <7.9 1.6 ± 0.5 C07
1632 1 –20.55 17.0 8.4 ± 4.4b 21.2a 698 ± 196 BVH <7.9 <1.9 C07
1684 –3 –16.41 17.0 10.8 ± 8.8 17.8 ± 2.9 2.2 ± 0.9 BVH <3.6
1706 –1 –11.35 17.0 13.8 ± 7.2 15.6a 0.041 ± 0.011 gi <3.6
1715 –1 –15.05 17.0 21.2 ± 8.1 15.6a 0.71 ± 0.46 BH <3.6

Notes.

(a)

The SED fit is done at fixed temperature.

(b)

The SED fit includes a synchrotron component.

(d)

This source could not be well observed by ALFALFA because of contamination from the M 87 radio continuum.

(e)

This source is outside the 4–16 deg declination strip observed by ALFALFA.

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