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Table 3:

Observational data - upper limits.
galaxy RA, Dec (2000) Optical Type Group $v_{\rm central}$ rms
name   size       noise
  h m s o arcmin $\hbox{$^{\prime\prime}$ }$ [arcmin]     [km s-1] [mJy]
d0224+4102 02 24 20.7 +41 02 12 $0.50 \times 0.30$ Ir N1023 650 3
d0237+4136 02 37 18.8 +41 36 07 $0.40 \times 0.35$ Ir N1023 650 3
d0241+3653 02 41 31.5 +36 52 27 $0.70 \times 0.40$ Ir N1023 650 3
d0243+3759 02 43 02.0 +37 59 26 $0.60 \times 0.50$ Sph N1023 650 3
d0246+3910 02 46 12.4 +39 10 55 $0.75 \times 0.50$ Ir N1023 650 3
d0246+3249 02 46 21.8 +32 49 45 $0.65 \times 0.35$ Ir N1023 650 3
d0246+3832 02 46 49.0 +38 32 51 $0.40 \times 0.25$ Ir N1023 650 3
d0921+5016 09 21 57.1 +50 16 12 $1.10 \times 0.90$ Sph N2841 650 4
d0926+7030 09 26 27.9 +70 30 24 $0.40 \times 0.40$ Ir M81 10 8
d1014+6845 10 14 55.8 +68 45 27 $0.20 \times 0.20$ Ir M81 10 6
d1018+4109 10 18 22.6 +41 09 58 $0.60 \times 0.40$ Ir N3180 570 3
d1028+7014 10 28 39.7 +70 14 01 $0.70 \times 0.45$ Sm M81 10 7
LeG10 10 43 55.4 +12 08 07 $0.15 \times 0.15$ Ir Leo I 700 5
LeG11 10 44 02.1 +15 35 20 $0.50 \times 0.45$ Ir Leo I 700 6
FS14, KK93 10 46 24.8 +14 01 30 $0.69 \times 0.55$ Ir Leo I 700 8
FS40, LeG19 10 49 37.1 +11 21 06 $0.60 \times 0.40$ Ir Leo I 700 7
UGC 5944 10 50 19.1 +13 16 19 $1.10 \times 1.05$ Sm Leo I 700 6
LeG28 10 53 00.7 +10 22 45 $0.60 \times 0.30$ Ir Leo I 700 5
d1058+2006 10 58 16.0 +20 06 26 $0.70 \times 0.50$ Ir N3507 980 2
LeG33 11 00 45.2 +14 10 20 $0.55 \times 0.30$ Ir Leo I 700 5
d1106+1250 11 06 10.5 +12 50 42 $0.50 \times 0.25$ Ir N3507 980 3
d1120+1332 11 20 16.1 +13 32 49 $0.60 \times 0.35$ Ir N3627 790 4
d1121+1830 11 21 53.8 +18 30 08 $0.35 \times 0.30$ Ir N3607 900 4
d1129+4606 11 29 25.0 +46 06 47 $0.70 \times 0.45$ Ir N3726 870 4
d1134+1709 11 34 16.2 +17 09 46 $0.70 \times 0.40$ Sm N3686 1150 4
d1140+4628 11 40 03.7 +46 28 42 $0.60 \times 0.50$ Sph N3726 780 5
d1142+5210 11 42 30.1 +52 10 36 $0.30 \times 0.25$ Ir? N3953 1050 5
d1148+5555 11 48 43.8 +55 55 45 $0.60 \times 0.45$ Ir N3953 1050 3
d1150+5546 11 50 06.3 +55 46 57 $1.00 \times 0.70$ Ir N3953 1050 3
d1154+3635 11 54 23.9 +36 35 04 $0.70 \times 0.60$ Ir N4062 780 3
d1156+5548 11 56 01.2 +55 48 46 $0.45 \times 0.30$ Ir N3953 1050 4
d1205+4342 12 05 25.0 +43 42 27 $0.80 \times 0.50$ Ir N4183 930 2
d1212+4237 12 12 18.0 +42 37 32 $0.50 \times 0.45$ Ir N4183 930 2
d1214+2749 12 14 42.3 +27 49 55 $0.35 \times 0.30$ Ir N4274 930 4
d1216+3353 12 16 28.8 +33 53 08 $0.60 \times 0.45$ Ir N4244 250 4
d1216+2928 12 16 39.2 +29 28 46 $0.30 \times 0.25$ Ir N4274 930 4
d1217+2914 12 17 47.2 +29 14 36 $0.40 \times 0.40$ Ir N4274 930 5
d1218+2838 12 18 29.4 +28 38 45 $0.80 \times 0.70$ Ir N4274 930 4
d1218+3003 12 18 31.8 +30 03 36 $0.70 \times 0.35$ Ir N4274 930 4
d1218+2938 12 18 43.6 +29 38 04 $0.40 \times 0.35$ Ir N4274 930 4
d1219+4743 12 19 06.5 +47 43 51 $0.60 \times 0.50$ Ir N4258 450 6
d1220+4700 12 20 40.6 +47 00 03 $0.30 \times 0.30$ dE N4258 450 6
d1221+2905 12 21 45.8 +29 05 02 $0.35 \times 0.30$ Ir? N4178 400 4
d1223+2832 12 23 09.5 +28 32 35 $0.30 \times 0.30$ Ir? N4278 650 4
d1224+4707 12 24 12.0 +47 07 24 $0.40 \times 0.35$ dE N4346 770 4
d1228+4358 12 28 44.9 +43 58 18 $4.00 \times 1.00$ Ir N4490 560 6
d1229+3056 12 29 41.2 +30 56 41 $0.40 \times 0.30$ Ir N4278 650 3
d1230+3002 12 30 25.8 +30 02 24 $0.55 \times 0.40$ Ir N4278 650 4
d1317+4423 13 17 19.5 +44 23 48 $0.80 \times 0.50$ Ir N5194 460 5
UGCA 361 13 32 36.2 +49 49 49 $1.20 \times 0.65$ Ir N5194 460 3
d1348+4335 13 48 57.6 +43 35 57 $0.70 \times 0.40$ Ir N5194 460 4
UGC 8882 13 57 14.6 +54 06 03 $1.10 \times 0.80$ Sph M101 250 8
d1504+5538 15 04 51.2 +55 38 42 $0.35 \times 0.30$ Ir N5906 670 5
d1508+5515 15 08 32.5 +55 15 48 $0.50 \times 0.40$ Ir N5906 670 5


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