Title: The Arecibo Legacy Fast ALFA Survey: V. HI Source Catalog of the Anti-Virgo Region at {delta} = +27 degrees Authors: Saintonge A., Giovanelli R., Haynes M.P., Hoffman G.L., Kent B.R., Martin A.M., Stierwalt S., Brosch N. Table: HI Candidate Detections ================================================================================ Byte-by-byte Description of file: datafile1.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- ID Source identification 7- 12 I6 --- AGC Arecibo General Catalog identification (1) 14- 15 I2 h HIRAh HI Hour of Right Ascension (J2000) (2) 17- 18 I2 min HIRAm HI Minute of Right Ascension (J2000) (2) 20- 23 F4.1 s HIRAs HI Second of Right Ascension (J2000) (2) 25 A1 --- HIDE- HI Declination sign (J2000) (2) 26- 27 I2 deg HIDEd HI Degree of Declination (J2000) (2) 29- 30 I2 arcmin HIDEm HI Arcminute of Declination (J2000) (2) 32- 33 I2 arcsec HIDEs HI Arcsecond of Declination (J2000) (2) 35- 36 I2 h ORAh ? Optical Hour of Right Ascension (J2000) (3) 38- 39 I2 min ORAm ? Optical Minute of Right Ascension (J2000) (3) 41- 44 F4.1 s ORAs ? Optical Second of Right Ascension (J2000) (3) 46 A1 --- ODE- Optical Declination sign (J2000)(3) 47- 48 I2 deg ODEd ? Optical Degree of Declination (J2000) (3) 50- 51 I2 arcmin ODEm ? Optical Arcminute of Declination (J2000) (3) 53- 54 I2 arcsec ODEs ? Optical Arcsecond of Declination (J2000) (3) 56- 60 I5 km/s cz Heliocentric velocity of the HI source (4) 62- 64 I3 km/s W50 Velocity width at 50% level (5) 66- 68 I3 km/s e_W50 Uncertainty in W50 70- 75 F6.2 Jy.km/s Fc Integrated flux density (6) 77- 80 F4.2 Jy.km/s e_Fc Uncertainty in Fc 82- 86 F5.1 --- S/N Signal-to-noise ratio of detection (7) 88- 91 F4.2 mJy rms Noise figure of spatially integrated spectral profile (8) 93- 97 F5.1 Mpc Dis ? Adopted distance (9) 99-103 F5.2 [solMass] logM ? Log of HI mass (10) 105-340 A236 --- Code Object code (11) -------------------------------------------------------------------------------- Note (1): The AGC entry normally corresponds to an optical counterpart except in the cases of HI sources which cannot be associated with an optical object with any high degree of probability. Note (2): Of the HI source, after correction for systematic telescope pointing errors, which are on the order of 20''. The accuracy of the HI positions depends on source strength. On average, the positional accuracy is about 19''. Note (3): Optical galaxy found to provide a reasonable optical counterpart. Quality of centroids is estimated to be 2\arcsec~ or better. The assessment of optical identification is based on spatial proximity, optical redshift (if available), morphology and color. For sources with no discernible optical counterpart and those for which such assignment is ambiguous, due to the presence of more than one equally possible optical counterpart, no optical position is listed. Note (4): Measured as the midpoint between the channels at which the flux density drops to 50% of each of the two peaks (or of one, if only one is present) at each side of the spectral feature. Note (5): This value is corrected for instrumental broadening. No corrections due to turbulent motions, disk inclination or cosmological effects are applied. Note (6): Measured on the integrated spectrum, obtained by spatially integrating the source image over a solid angle of at least 7' X 7' and dividing by the sum of the survey beam values over the same set of image pixels. Note (7): Estimated as S/N = (1000Fc/W50)(w_smo_^1/2^/rms). Where w_smo_ is either W50/(2X 10) for W50 < 400 km/s or 400/(2X 10) = 20 for W50 {>=} 400 km/s [w_smo_ is a smoothing width expressed as the number of spectral resolution bins of 10 km/s bridging half of the signal width]. Note (8): The rms as measured over the signal- and rfi-free portions of the spectrum, after Hanning smoothing to a spectral resolution of 10 km/s. Note (9): For objects with cz > 6000 km/s, the distance is simply cz_cmb_/H_o_; cz_cmb_ is the recession velocity measured in the Cosmic Microwave Background reference frame and H_o_ is the Hubble constant, for which we use a value of 70 km/s/Mpc. For objects of lower cz_cmb_, we use the peculiar velocity model for the local universe of Masters (2005), which is based on data from the SFI++ catalog of galaxies (Springob et al. 2007). Note (10): Obtained by using the expression M_HI_ = 2.356e5 Dis^2^ Fc. Note (11): 1 = refers to sources of S/N and general qualities that make it a reliable detection. See text for additional details. 2 = refers to sources of low S/N (< 6.5), which would ordinarily not be considered reliable detections by the criteria set for code 1. 9 = refers to objects assumed to be HVCs; no estimate of their distances is made. * = Additional comments for source from text provided. -------------------------------------------------------------------------------- 2- 1 331405 00 00 03.7 +26 00 56 00 00 03.5 +26 00 50 10409 316 8 2.35 0.08 15.7 1.88 143.8 10.06 1 2- 2 102571 00 00 17.2 +27 23 59 00 00 17.3 +27 24 03 4654 104 3 1.83 0.06 19.0 2.10 65.9 9.27 1 2- 3 12896 00 00 30.1 +26 19 28 00 00 31.4 +26 19 31 7653 170 10 2.82 0.08 22.0 2.20 104.5 9.86 1 2- 4 102576 00 00 35.3 +26 27 12 -430 21 2 0.58 0.03 11.7 2.40 9 * 2- 4: compact HVC; one of two nearby knots (the other is AGC102578, another HVC from this catalog) 2- 5 102578 00 00 42.3 +26 33 11 -429 22 3 0.64 0.04 12.8 2.32 9 * 2- 5: compact HVC; one of two nearby knots (the other is AGC102576, another HVC from this catalog) 2- 6 12920 00 02 23.1 +27 12 51 00 02 23.0 +27 12 38 7613 281 2 2.60 0.09 16.0 2.17 103.9 9.82 1 2- 7 102553 00 03 23.1 +27 24 29 00 03 25.1 +27 24 11 4544 83 10 0.79 0.05 9.3 2.08 64.3 8.89 1 2- 8 100025 00 04 43.9 +26 50 16 00 04 44.5 +26 49 57 7556 134 15 0.98 0.06 9.8 1.93 103.1 9.39 1 2- 9 102554 00 05 15.7 +27 29 19 00 05 15.3 +27 29 23 11854 232 27 1.55 0.08 11.0 2.06 164.5 10.00 1 2- 10 102555 00 05 17.4 +26 31 19 00 05 19.2 +26 31 10 7432 140 33 0.68 0.06 7.0 1.85 101.3 9.22 1 2- 11 40 00 05 49.2 +27 26 57 00 05 48.4 +27 26 56 7522 388 2 2.28 0.10 12.8 2.02 102.6 9.75 1 2- 12 100037 00 06 03.0 +27 20 52 00 06 02.5 +27 20 58 3182 63 1 1.14 0.04 16.5 1.94 44.8 8.73 1 2- 13 102556 00 06 07.5 +26 05 37 00 06 08.5 +26 06 44 7288 261 67 1.19 0.09 8.1 2.03 99.3 9.44 1 2- 14 102557 00 06 25.3 +27 55 00 00 06 25.4 +27 54 40 7527 270 49 1.56 0.09 10.6 2.00 102.7 9.59 1 2- 15 50 00 06 40.0 +26 09 09 00 06 40.1 +26 09 14 7556 401 14 2.63 0.09 16.0 1.83 103.1 9.82 1 2- 16 102558 00 07 03.6 +27 00 33 00 07 04.6 +27 01 28 2963 48 2 0.44 0.04 7.3 1.92 41.7 8.26 1 2- 17 57 00 07 15.9 +27 42 50 00 07 15.9 +27 42 28 4550 318 1 9.59 0.08 63.3 1.90 64.2 9.97 1 2- 18 59 00 07 20.1 +27 40 31 00 07 17.1 +27 40 40 7559 381 0 2.04 0.10 11.5 2.02 103.2 9.71 1 2- 19 102559 00 07 48.7 +27 30 06 00 07 49.0 +27 30 32 7518 166 11 0.95 0.07 8.2 2.02 102.6 9.37 1 2- 20 102560 00 08 05.0 +26 05 51 00 08 05.2 +26 06 03 11707 151 6 1.66 0.07 13.8 2.19 162.4 10.01 1 2- 21 69 00 08 11.8 +27 31 53 00 08 10.9 +27 31 39 4637 175 1 6.71 0.07 54.7 2.07 65.5 9.83 1 2- 22 102561 00 08 58.0 +26 13 56 00 08 56.3 +26 14 19 4405 97 11 0.88 0.05 10.0 1.98 62.1 8.90 1 2- 23 102562 00 09 31.1 +26 20 08 00 09 30.0 +26 20 02 11693 223 5 1.36 0.08 9.6 2.12 162.2 9.93 1 2- 24 86 00 09 48.6 +27 50 02 00 09 48.2 +27 49 55 8312 359 2 3.40 0.10 18.5 2.18 114.0 10.02 1 2- 25 102563 00 10 19.8 +27 45 49 00 10 22.2 +27 45 28 7321 150 6 0.99 0.07 8.7 2.07 99.8 9.37 1 2- 26 102564 00 10 49.2 +26 26 06 00 10 49.2 +26 26 02 11720 313 3 2.41 0.10 13.8 2.21 162.6 10.18 1 2- 27 102565 00 11 15.4 +26 54 06 00 11 17.3 +26 54 02 11804 286 7 1.10 0.09 7.4 1.97 163.8 9.84 1 2- 28 101105 00 11 26.9 +27 47 12 00 11 27.8 +27 47 25 7394 308 6 1.70 0.10 10.0 2.16 100.9 9.61 1 2- 29 107 00 11 38.0 +27 58 14 00 11 38.1 +27 56 52 7437 387 5 1.52 0.09 8.7 1.99 101.5 9.57 1 2- 30 110 00 12 00.7 +26 23 52 00 12 01.3 +26 23 35 4507 176 6 2.96 0.07 26.4 1.88 63.5 9.45 1 2- 31 100080 00 12 10.0 +27 54 33 00 12 09.3 +27 54 35 7396 327 12 1.95 0.10 11.5 2.10 100.9 9.67 1 2- 32 127 00 13 57.5 +26 58 04 00 13 56.5 +26 58 03 4683 198 1 7.55 0.07 58.4 2.05 66.0 9.89 1 2- 33 100101 00 14 55.5 +26 19 43 00 14 54.8 +26 19 53 7358 146 3 3.41 0.06 30.2 2.09 100.3 9.91 1 2- 34 102566 00 14 56.2 +26 16 11 00 14 57.7 +26 15 49 7384 87 2 2.13 0.05 27.1 1.87 100.7 9.71 1 * 2- 34: just south of AGC100101(001454.8+261953), may be interacting (this signal may be contaminated by the other) 2- 35 102245 00 15 37.3 +27 14 05 00 15 36.6 +27 14 26 7336 344 22 2.52 0.09 16.2 1.88 100.0 9.77 1 2- 36 102567 00 15 41.9 +27 15 23 00 15 42.6 +27 15 10 7431 110 3 1.17 0.06 12.4 2.01 101.4 9.45 1 * 2- 36: close companion of AGC102245(001536.6+271426); blend: HI signals difficult to untangle 2- 37 100124 00 16 26.3 +27 34 07 00 16 25.8 +27 34 25 4595 100 0 0.98 0.05 10.6 2.05 64.7 8.99 1 2- 38 157 00 16 52.7 +27 51 26 00 16 53.8 +27 50 52 9089 125 15 0.99 0.07 9.6 2.05 125.1 9.56 1 2- 39 101815 00 17 14.1 +27 15 08 00 17 13.3 +27 14 54 3704 152 6 1.77 0.06 16.4 1.95 51.9 9.05 1 2- 40 102246 00 17 17.1 +26 51 45 00 17 18.3 +26 51 41 8911 132 30 1.22 0.06 12.1 1.96 122.5 9.64 1 * 2- 40: parameters uncertain, signal merging with strong rfi 2- 41 100141 00 17 30.3 +26 15 50 00 17 30.2 +26 15 33 7463 163 6 1.08 0.06 10.0 1.88 101.8 9.42 1 2- 42 102247 00 18 08.4 +26 58 45 00 18 06.3 +26 58 52 4744 61 6 0.56 0.05 8.0 2.03 66.8 8.77 1 * 2- 42: possible alternative opt.id with 001805.8+265933, but farther from HI center and LSB 2- 43 101791 00 19 05.8 +26 37 28 00 19 05.8 +26 37 33 11650 315 9 2.08 0.10 12.2 2.16 161.7 10.11 1 2- 44 102248 00 19 50.0 +27 28 59 00 19 49.3 +27 28 47 12782 116 5 0.87 0.07 7.8 2.30 177.9 9.81 1 2- 45 100176 00 21 09.8 +26 30 23 00 21 06.6 +26 30 48 11653 351 28 0.83 0.10 4.6 2.16 161.7 9.71 2 2- 46 101816 00 21 15.2 +26 23 07 00 21 15.3 +26 23 07 9178 171 7 1.21 0.07 10.0 2.06 126.4 9.66 1 2- 47 102249 00 22 10.4 +27 02 58 00 22 09.1 +27 02 38 9407 176 9 1.13 0.08 9.8 1.94 129.6 9.65 1 * 2- 47: possible alternative opt.id with 002204.3+270221, 002211.6+270115 but farther from HI center 2- 48 102252 00 22 28.5 +27 10 28 00 22 28.6 +27 10 23 9445 150 4 0.75 0.08 6.1 2.25 130.2 9.48 1 2- 49 102294 00 22 55.2 +26 07 33 00 22 54.0 +26 07 20 7331 255 10 1.04 0.08 7.1 2.04 100.0 9.39 1 * 2- 49: possible alternative opt.id with 002255.0+260751 2- 50 221 00 23 12.5 +27 26 09 00 23 10.9 +27 25 55 3904 149 0 1.84 0.07 15.9 2.12 54.6 9.11 1 2- 51 102255 00 28 12.9 +26 12 36 00 28 14.7 +26 12 43 10264 222 6 0.98 0.08 6.6 2.22 141.9 9.67 1 2- 52 278 00 28 21.5 +27 21 59 00 28 21.2 +27 22 08 9591 381 5 2.87 0.10 16.7 1.97 132.3 10.07 1 2- 53 102297 00 29 27.4 +27 10 43 00 29 28.2 +27 10 47 16563 237 25 1.31 0.09 8.6 2.22 231.9 10.22 1 * 2- 53: opt.id ambiguous; other possible counterpart at 002930.1+271056 but farther from HI center 2- 54 102289 00 29 38.9 +27 01 39 00 29 36.3 +27 01 47 6933 62 7 0.50 0.05 6.7 2.09 94.4 9.02 1 2- 55 102257 00 29 47.2 +27 12 12 00 29 46.8 +27 12 56 9602 213 4 1.32 0.09 8.2 2.45 132.5 9.74 1 2- 56 102258 00 30 03.0 +26 34 13 00 30 02.6 +26 34 11 8176 301 2 1.34 0.09 8.0 2.15 112.1 9.60 1 2- 57 101819 00 30 27.2 +26 38 46 00 30 26.8 +26 38 33 9665 261 5 2.35 0.08 16.4 1.97 133.4 9.99 1 2- 58 101820 00 30 51.9 +27 23 36 00 30 51.4 +27 23 24 11259 164 17 0.76 0.07 6.5 2.04 156.2 9.64 2 2- 59 102579 00 31 54.7 +26 30 45 -302 25 2 0.78 0.04 12.9 2.70 9 * 2- 59: compact HVC; near several other compact clouds 2- 60 102259 00 32 36.5 +26 29 33 00 32 36.1 +26 29 36 9017 106 8 0.69 0.06 7.5 2.00 124.1 9.40 1 2- 61 102260 00 34 04.9 +26 19 05 00 34 04.4 +26 18 17 7199 161 6 1.06 0.07 8.9 2.10 98.2 9.38 1 2- 62 102580 00 34 21.4 +27 58 41 -150 27 1 4.14 0.10 24.8 7.10 9 * 2- 62: HVC; close in frequency to Galactic HI, but appears distinct 2- 63 102261 00 35 41.4 +26 37 03 00 35 44.4 +26 36 57 10082 215 23 0.91 0.08 7.1 1.95 139.4 9.62 1 2- 64 102262 00 36 29.9 +26 54 10 00 36 29.6 +26 54 17 5222 147 9 0.73 0.07 6.3 2.12 73.3 8.97 1 2- 65 102582 00 37 34.7 +26 36 49 -368 26 2 0.75 0.04 11.7 2.77 9 * 2- 65: compact HVC; near several other compact clouds 2- 66 101821 00 38 34.2 +26 20 56 00 38 32.3 +26 20 50 7183 151 18 0.77 0.06 6.7 2.07 98.0 9.24 1 2- 67 100381 00 38 58.3 +26 57 58 00 38 56.1 +26 57 50 5171 217 3 1.73 0.07 13.0 2.02 72.5 9.33 1 2- 68 102263 00 39 18.0 +26 45 28 00 39 19.6 +26 45 42 9942 226 20 0.99 0.09 6.2 2.39 137.4 9.64 1 2- 69 102299 00 39 28.4 +26 04 38 00 39 27.8 +26 04 29 5271 59 12 0.54 0.05 7.7 2.05 73.9 8.84 1 * 2- 69: possible alternative opt.id with 003928.9+260506, but farther from HI center 2- 70 102265 00 39 29.5 +27 43 14 00 39 29.4 +27 43 03 7236 240 34 0.81 0.07 6.1 1.92 98.8 9.27 1 2- 71 102583 00 39 41.9 +26 05 20 -378 33 2 2.22 0.06 25.2 3.43 9 * 2- 71: HVC; part of a stream of clouds 2- 72 102584 00 40 25.7 +26 14 58 -341 25 1 2.30 0.05 34.6 2.94 9 * 2- 72: HVC; part of a stream of clouds 2- 73 102585 00 40 28.9 +27 42 21 -366 24 1 1.26 0.04 19.3 2.92 9 * 2- 73: HVC; in a complex of compact clouds 2- 74 101822 00 40 35.9 +27 03 03 00 40 36.4 +27 03 02 5129 132 2 3.04 0.06 31.4 1.89 71.9 9.57 1 2- 75 102266 00 40 42.5 +26 01 25 00 40 42.5 +26 01 47 5318 175 4 1.23 0.06 10.8 1.92 74.6 9.21 1 2- 76 102586 00 41 07.6 +26 29 33 -337 23 2 2.24 0.05 29.3 3.53 9 * 2- 76: HVC; part of a stream of clouds 2- 77 101823 00 41 13.6 +27 21 56 00 41 13.0 +27 22 20 10338 307 7 1.94 0.09 12.3 2.01 143.1 9.97 1 2- 78 102587 00 41 55.0 +27 33 03 -375 24 1 4.43 0.07 42.7 4.69 9 * 2- 78: HVC; in a complex of compact clouds 2- 79 102267 00 42 19.6 +27 09 51 00 42 20.4 +27 09 50 5254 25 4 0.38 0.03 8.0 2.14 73.7 8.69 1 2- 80 100482 00 42 57.3 +27 15 08 00 42 57.9 +27 15 12 5286 230 4 2.96 0.07 22.6 1.93 74.1 9.58 1 2- 81 100489 00 43 57.2 +26 08 42 00 43 57.8 +26 08 49 4898 39 1 0.80 0.04 15.2 1.87 68.5 8.95 1 2- 82 469 00 44 04.5 +26 12 04 00 44 03.7 +26 12 27 10083 533 14 2.47 0.12 10.0 2.07 139.4 10.05 1 2- 83 102269 00 44 13.9 +26 37 50 00 44 13.4 +26 37 30 5335 100 1 0.75 0.06 7.6 2.20 74.8 9.00 1 2- 84 470 00 44 14.4 +26 50 35 00 44 12.5 +26 50 45 5188 255 2 10.42 0.09 70.3 2.07 72.7 10.11 1 2- 85 100499 00 44 57.4 +27 26 59 00 44 56.8 +27 27 02 5186 122 9 1.48 0.06 14.5 2.05 72.6 9.27 1 2- 86 102273 00 46 25.0 +27 04 28 00 46 21.5 +27 04 31 10329 64 10 0.50 0.06 6.5 2.17 143.0 9.38 1 2- 87 101825 00 46 28.2 +26 41 28 00 46 27.7 +26 41 31 5085 62 4 0.48 0.05 6.0 2.30 71.1 8.76 2 2- 88 102588 00 46 42.8 +26 53 06 -343 28 2 2.67 0.09 21.1 5.29 9 * 2- 88: HVC; one of the knots in a complex that extends over 1.5 degrees 2- 89 100550 00 46 49.3 +27 56 33 00 46 47.0 +27 56 30 6874 275 4 1.28 0.09 8.3 2.08 93.7 9.42 1 2- 90 483 00 46 51.9 +26 28 36 00 46 50.3 +26 28 34 4951 235 6 2.44 0.08 17.5 2.03 69.2 9.44 1 2- 91 102589 00 47 07.3 +27 29 24 -340 28 1 2.45 0.06 26.0 3.97 9 * 2- 91: HVC; one of the knots in a complex that extends over 1.5 degrees 2- 92 489 00 47 20.2 +27 50 00 00 47 18.6 +27 49 38 4740 303 0 2.17 0.08 15.0 1.86 66.1 9.35 1 2- 93 102274 00 47 20.4 +26 01 41 00 47 20.4 +26 01 47 4702 127 23 1.31 0.06 13.6 1.90 65.6 9.12 1 2- 94 101826 00 47 37.3 +26 48 04 00 47 37.7 +26 48 19 4954 114 5 1.53 0.06 15.5 2.05 69.2 9.24 1 2- 95 102590 00 47 47.5 +26 51 45 -337 25 1 0.92 0.04 15.5 2.62 9 * 2- 95: HVC; one of the knots in a complex that extends over 1.5 degrees 2- 96 491 00 48 03.0 +27 37 26 00 48 01.4 +27 37 29 4938 553 26 3.00 0.10 13.4 1.81 69.0 9.53 1 2- 97 100572 00 48 13.2 +27 59 25 00 48 13.2 +27 59 19 7020 265 0 1.30 0.08 9.1 1.95 95.8 9.45 1 2- 98 100573 00 48 18.2 +26 27 13 00 48 16.6 +26 28 02 5269 162 11 0.65 0.07 5.4 2.13 73.8 8.92 2 2- 99 497 00 48 34.8 +27 41 23 00 48 34.6 +27 41 36 5213 177 15 2.96 0.07 25.3 1.96 72.9 9.57 1 2-100 102275 00 49 13.4 +27 37 10 00 49 13.9 +27 36 46 7056 245 12 1.32 0.07 10.0 1.90 96.3 9.46 1 2-101 101827 00 50 11.9 +27 13 21 00 50 12.2 +27 13 25 4935 115 8 1.00 0.06 10.3 2.02 68.9 9.05 1 2-102 102278 00 50 18.3 +27 29 14 00 50 18.8 +27 28 17 10159 130 24 0.85 0.07 8.2 2.04 140.6 9.60 1 2-103 102279 00 51 01.7 +26 01 08 00 51 02.0 +26 00 40 10241 225 36 1.10 0.08 8.2 1.99 141.7 9.72 1 2-104 101828 00 51 25.9 +27 16 37 00 51 24.7 +27 16 01 4526 40 9 0.53 0.04 8.7 2.13 62.9 8.69 1 2-105 535 00 52 30.3 +26 08 10 00 52 31.5 +26 07 57 14797 217 12 1.74 0.08 12.0 2.20 206.8 10.24 1 2-106 102280 00 52 33.8 +27 07 08 00 52 34.6 +27 06 41 11462 71 3 0.69 0.05 9.1 2.01 159.2 9.62 1 2-107 102281 00 52 42.0 +27 23 12 00 52 40.8 +27 23 10 6851 127 4 0.75 0.06 7.4 1.99 93.4 9.19 1 2-108 102283 00 53 48.9 +27 03 39 00 53 46.6 +27 03 48 10129 126 44 0.96 0.08 8.7 2.20 140.2 9.65 1 2-109 102591 00 54 24.7 +27 08 10 -359 22 2 1.43 0.06 18.2 3.69 9 * 2-109: compact HVC; in the vicinity of other clouds 2-110 102284 00 54 32.0 +26 34 50 00 54 31.1 +26 35 00 14563 157 13 0.90 0.08 7.3 2.22 203.5 9.94 1 2-111 102592 00 57 39.7 +27 30 13 -390 25 1 1.81 0.04 29.2 2.77 9 * 2-111: HVC; part of the Western end of Wright's Cloud 2-112 102593 00 58 27.8 +27 55 37 -394 26 1 8.01 0.06 94.1 3.67 9 * 2-112: HVC; part of the Western end of Wright's Cloud 2-113 102569 00 58 29.5 +27 45 21 00 58 29.3 +27 45 28 10930 180 22 1.29 0.07 11.2 1.92 151.7 9.85 1 2-114 102570 00 59 27.8 +26 15 08 00 59 25.4 +26 15 35 9598 129 29 0.83 0.06 8.5 1.93 132.6 9.54 1 2-115 100705 01 00 30.2 +27 01 46 01 00 27.8 +27 01 30 14914 156 32 0.65 0.07 5.2 2.26 208.6 9.82 2 2-116 101685 01 00 33.3 +27 05 51 01 00 34.0 +27 05 53 11040 195 8 1.92 0.08 14.3 2.15 153.3 10.03 1 2-117 113757 01 00 42.4 +27 42 37 -392 30 1 1.66 0.06 20.6 3.27 9 * 2-117: HVC; part of the Western end of Wright's Cloud 2-118 113758 01 00 55.1 +26 03 46 -386 22 4 0.44 0.04 7.6 2.75 9 * 2-118: HVC; compact cloud, West of the Southern extension of Wright's Cloud 2-119 100714 01 01 57.1 +26 29 00 01 01 58.4 +26 29 12 10064 69 13 0.58 0.05 8.0 1.93 139.3 9.42 1 2-120 113759 01 02 10.9 +27 00 04 -397 27 1 0.72 0.05 10.6 2.90 9 * 2-120: HVC; one knot of a small cloud, just West of the Southern extension of Wright's Cloud 2-121 100719 01 02 24.4 +26 37 05 01 02 24.0 +26 37 17 4994 221 19 1.64 0.08 12.1 2.04 69.5 9.27 1 2-122 113760 01 02 39.4 +26 56 13 -397 28 4 0.75 0.05 12.3 2.56 9 * 2-122: HVC; one knot of a small cloud, just West of the Southern extension of Wright's Cloud 2-123 113761 01 02 46.2 +27 07 07 -405 25 1 0.44 0.04 8.0 2.45 9 * 2-123: HVC; one knot of a small cloud, just West of the Southern extension of Wright's Cloud 2-124 113747 01 03 17.5 +26 38 46 01 03 17.8 +26 38 16 14409 118 12 0.65 0.06 7.0 1.89 201.4 9.79 1 * 2-124: possible alternative opt.id with 010312.9+263826, but farther from HI center 2-125 112506 01 03 18.8 +26 47 58 01 03 17.8 +26 47 47 5054 128 10 1.27 0.06 12.4 2.02 70.4 9.17 1 2-126 112507 01 04 56.6 +26 49 33 01 04 56.5 +26 49 36 14258 196 39 1.28 0.07 10.2 1.99 199.3 10.08 1 2-127 113748 01 05 34.9 +27 30 36 01 05 36.9 +27 30 44 14218 184 26 0.94 0.08 7.8 1.99 198.7 9.94 1 2-128 113749 01 05 46.6 +26 55 28 01 05 45.3 +26 55 47 10115 376 51 1.30 0.11 6.5 2.29 140.1 9.78 1 2-129 113762 01 06 03.3 +27 15 33 -422 26 1 5.40 0.08 53.3 4.39 9 * 2-129: HVC; part of the southern extension of Wright's Cloud 2-130 113763 01 06 46.1 +27 58 08 -408 24 1 20.64 0.09 193.9 4.81 9 * 2-130: HVC; part of the southern extension of Wright's Cloud 2-131 112508 01 07 01.3 +26 31 00 01 07 00.8 +26 30 54 10130 167 28 1.00 0.07 8.8 1.95 140.3 9.67 1 2-132 113766 01 07 55.8 +26 57 06 -421 20 2 33.32 0.09 312.6 5.31 9 * 2-132: HVC; part of the southern extension of Wright's Cloud 2-133 113767 01 08 12.2 +27 31 54 -420 26 1 18.59 0.13 139.0 5.76 9 * 2-133: HVC; part of the southern extension of Wright's Cloud 2-134 113768 01 08 20.0 +26 38 04 -421 22 1 27.11 0.11 242.8 5.21 9 * 2-134: HVC; part of the southern extension of Wright's Cloud 2-135 113770 01 09 24.0 +26 04 53 -427 22 2 24.49 0.09 235.7 4.89 9 * 2-135: HVC; part of the southern extension of Wright's Cloud 2-136 113790 01 12 59.7 +27 38 00 01 13 02.1 +27 38 13 4952 31 10 0.33 0.03 6.6 1.98 68.7 8.57 1 * 2-136: possible alternative opt.id with 011257.2+273801 2-137 113750 01 13 10.7 +27 48 04 01 13 09.3 +27 48 04 13562 91 5 0.68 0.06 7.3 2.18 189.4 9.76 1 2-138 110150 01 14 45.2 +27 08 20 01 14 45.5 +27 08 06 3617 108 1 4.71 0.06 49.9 2.02 49.5 9.44 1 2-139 113773 01 14 47.7 +27 42 19 -360 20 1 0.73 0.04 12.8 2.83 9 * 2-139: compact HVC; in the vicinity of other clouds 2-140 112511 01 16 43.1 +26 55 17 01 16 43.0 +26 54 45 12277 102 7 0.74 0.06 7.6 2.14 171.1 9.71 1 2-141 112512 01 17 40.6 +27 00 51 01 17 42.4 +27 00 33 12127 150 2 1.81 0.07 15.9 2.08 169.0 10.09 1 2-142 113751 01 17 42.3 +26 57 58 01 17 41.1 +26 57 47 16099 83 5 0.63 0.06 6.7 2.30 225.7 9.88 1 2-143 113752 01 18 03.3 +27 11 13 01 18 05.5 +27 11 17 12427 91 7 0.71 0.06 7.7 2.14 173.3 9.70 1 2-144 113774 01 18 05.4 +27 32 36 -320 27 2 1.10 0.06 14.4 3.26 9 * 2-144: compact HVC; interesting morphology, a string of knots 2-145 113775 01 20 32.1 +26 26 58 -148 27 2 0.88 0.05 11.0 3.40 9 * 2-145: HVC; close in frequency to Galactic HI, yet seems to be spectrally distinct 2-146 113753 01 21 02.7 +26 05 17 01 21 02.1 +26 05 20 3103 41 4 0.49 0.04 8.5 2.02 42.2 8.31 1 2-147 110264 01 22 42.1 +26 52 43 01 22 43.1 +26 52 00 9069 245 7 1.73 0.08 11.6 2.13 125.3 9.81 1 * 2-147: HI signal most likely a blend of AGC110263(012240.8+265206) and AGC110264(012243.1+265200) (assigned to the latter due to better match with optical velocity). Signal also merges with strong rfi so parameters are uncertain 2-148 948 01 24 03.6 +27 02 58 01 24 04.1 +27 02 46 4916 166 11 2.20 0.07 18.4 2.07 68.0 9.38 1 2-149 110324 01 26 07.1 +27 57 54 01 26 08.8 +27 57 56 4019 85 4 0.64 0.05 7.7 2.01 55.0 8.66 1 * 2-149: possible alternative opt.id with 012608.7+275819, close companion 2-150 113755 01 27 55.2 +27 27 33 01 27 54.8 +27 27 19 9148 185 5 1.10 0.08 8.2 2.18 126.5 9.62 1 2-151 112515 01 29 45.0 +27 23 01 01 29 43.6 +27 23 40 12643 143 9 1.71 0.07 15.3 2.09 176.5 10.10 1 * 2-151: opt.id ambiguous; possible alternative opt.id with 012946.1+272221 (IRAS sources, cz=12566km/s) 2-152 112516 01 31 53.1 +27 19 56 01 31 54.0 +27 19 45 3820 30 4 0.46 0.05 8.9 2.11 52.1 8.47 2 2-153 112518 01 33 15.6 +26 15 07 01 33 15.6 +26 14 55 6952 296 3 2.72 0.08 18.1 1.95 95.2 9.76 1 2-154 112519 01 33 37.7 +26 25 16 01 33 39.2 +26 25 13 11093 241 37 1.08 0.09 6.9 2.23 154.4 9.78 1 2-155 110443 01 37 16.2 +26 26 03 01 37 15.2 +26 26 10 3875 61 1 0.91 0.04 12.4 2.10 52.8 8.78 1 2-156 112520 01 37 44.0 +27 10 50 01 37 43.7 +27 10 50 11085 353 17 1.96 0.11 10.6 2.19 154.3 10.04 1 2-157 113291 01 38 34.6 +26 37 46 01 38 35.9 +26 38 01 7132 167 23 1.06 0.07 9.3 1.97 97.8 9.38 1 2-158 112521 01 41 06.4 +27 19 03 01 41 08.0 +27 19 20 274 26 1 0.65 0.04 13.1 2.18 4.6 6.50 1 * 2-158: distance estimated at 7.2 Mpc based on membership of the NGC672 group 2-159 110477 01 41 46.4 +27 30 04 01 41 46.4 +27 30 12 10840 205 10 1.06 0.08 8.1 2.05 150.9 9.76 1 2-160 110482 01 42 16.8 +26 21 58 01 42 17.3 +26 22 00 357 30 2 1.24 0.04 23.2 2.14 5.6 6.96 1 * 2-160: distance estimated at 7.2 Mpc based on membership of the NGC672 group (Huchtmeier et al. 2000) 2-161 113295 01 43 40.5 +26 49 03 01 43 42.3 +26 49 03 13319 70 15 0.62 0.05 8.0 2.08 186.3 9.71 1 2-162 113294 01 43 46.3 +27 03 42 01 43 45.9 +27 03 47 11122 168 17 0.80 0.07 6.8 2.00 154.9 9.66 1 2-163 110790 01 44 29.8 +27 55 41 01 44 28.8 +27 55 44 4037 190 1 7.25 0.07 59.4 1.98 55.1 9.71 1 2-164 111945 01 44 42.4 +27 17 17 01 44 42.7 +27 17 18 423 36 1 2.80 0.04 48.2 2.15 6.4 7.43 1 * 2-164: distance estimated at 7.2 Mpc based on membership of the NGC672 group (Huchtmeier et al. 2000) 2-165 113296 01 44 46.1 +26 09 25 01 44 44.1 +26 09 06 16436 353 100 1.70 0.11 8.7 2.32 230.8 10.33 1 2-166 111946 01 46 42.3 +26 48 06 01 46 42.2 +26 48 05 367 21 3 0.72 0.03 15.4 2.23 5.7 6.74 1 * 2-166: distance estimated at 7.2 Mpc based on membership of the NGC672 group (Huchtmeier et al. 2000) 2-167 1250 01 47 24.6 +27 53 10 01 47 25.0 +27 53 09 3697 437 5 4.48 0.10 23.1 1.99 50.2 9.43 1 2-168 1249 01 47 30.0 +27 21 07 01 47 29.9 +27 19 58 330 115 3 88.51 0.08 719.9 2.56 5.2 8.76 1 * 2-168: parameters uncertain, signal partly blended with NGC672. Primary distance measurement of 7.2 Mpc (Karachentsev et al. 2004). 2-169 1256 01 47 53.9 +27 25 35 01 47 53.9 +27 25 55 429 205 2 111.02 0.09 696.2 2.49 6.5 9.04 1 * 2-169: parameters uncertain, signal partly blended with IC1727. Primary distance measurement of 7.2 Mpc (Karachentsev et al. 2004). 2-170 110534 01 48 33.5 +27 33 25 01 48 35.3 +27 33 24 10863 117 10 2.10 0.07 19.7 2.20 151.3 10.05 1 * 2-170: opt.id ambiguous; possible counterparts at AGC110534(014835.3+273324), AGC110535(014835.2+273253); HI signal probably a blend of these two very nearby spirals. Opt.id made based on best coordinate match and later morphology. 2-171 113756 01 48 42.9 +27 17 24 01 48 46.3 +27 17 20 10820 78 14 0.58 0.05 7.0 2.09 150.7 9.49 1 2-172 110543 01 49 20.6 +27 42 31 01 49 20.1 +27 42 44 10753 253 8 1.59 0.08 11.1 2.02 149.7 9.92 1 2-173 113298 01 49 57.6 +26 41 10 01 49 57.7 +26 40 59 3680 89 25 0.87 0.07 10.0 2.06 49.9 8.71 1 2-174 1291 01 50 13.4 +27 11 50 01 50 12.5 +27 11 45 3503 218 2 6.18 0.08 42.5 2.20 47.4 9.52 1 2-175 1292 01 50 13.9 +27 38 54 01 50 14.0 +27 38 45 3535 478 3 12.91 0.11 55.2 2.18 47.9 9.84 1 2-176 112523 01 50 49.7 +27 17 28 01 50 46.6 +27 16 41 14577 441 20 1.34 0.12 6.2 2.20 204.4 10.12 2 2-177 112524 01 51 47.9 +27 45 31 01 51 52.7 +27 45 31 10722 44 9 0.76 0.05 12.1 2.11 149.3 9.60 1 2-178 112526 01 54 38.3 +27 11 16 01 54 40.0 +27 11 10 8424 293 25 1.00 0.09 5.8 2.25 116.5 9.51 2 2-179 112525 01 54 39.9 +27 49 11 01 54 38.9 +27 49 19 14848 200 24 1.54 0.08 10.8 2.25 208.3 10.20 1 2-180 111977 01 55 21.1 +27 56 56 01 55 20.2 +27 57 14 207 29 3 0.78 0.05 14.2 2.29 3.7 6.39 1 * 2-180: primary distance measurement of 4.7 Mpc (Karachentsev et al. 2003). 2-181 112527 01 55 35.2 +27 43 31 01 55 35.6 +27 43 28 8345 99 5 1.45 0.05 16.5 1.97 115.4 9.66 1 2-182 113299 01 56 26.8 +27 40 48 01 56 25.2 +27 41 09 12699 240 11 1.31 0.09 8.4 2.25 177.6 9.99 1 2-183 112528 01 57 52.0 +26 45 55 01 57 52.2 +26 45 43 12421 257 6 2.63 0.08 19.0 1.92 173.6 10.27 1 2-184 113301 01 58 13.9 +27 53 11 01 58 14.4 +27 52 55 10401 192 2 1.56 0.07 13.1 1.92 144.8 9.89 1 2-185 113302 01 58 33.1 +27 49 45 01 58 31.6 +27 49 35 12305 174 18 0.93 0.08 7.2 2.20 172.0 9.81 1 2-186 112529 01 58 58.0 +26 57 40 01 58 59.6 +26 57 49 13035 56 5 0.98 0.05 13.0 2.23 182.4 9.89 1 2-187 112459 01 59 19.4 +27 00 51 01 59 19.2 +27 00 44 5306 130 3 1.08 0.06 10.7 1.99 73.4 9.14 1 2-188 110716 01 59 38.7 +27 25 41 01 59 38.1 +27 26 01 5269 205 2 3.01 0.08 22.4 2.10 72.8 9.58 1 2-189 112530 01 59 53.3 +26 23 58 01 59 51.8 +26 24 18 5239 164 20 1.92 0.06 18.4 1.82 72.4 9.38 1 * 2-189: opt.id ambiguous: possible alternative opt.id with AGC112531(015954.1+262401,no previous cz) 2-190 1507 02 01 30.1 +26 28 56 02 01 30.8 +26 28 51 5152 524 20 4.56 0.11 18.9 2.06 71.1 9.74 1 2-191 1510 02 01 45.6 +26 32 58 02 01 46.3 +26 32 46 5009 184 25 4.51 0.07 36.8 2.01 69.0 9.70 1 * 2-191: parameters uncertain, signal may be partly blended with UGC1507 2-192 1533 02 02 47.9 +26 34 55 02 02 48.1 +26 34 52 14595 231 6 2.30 0.09 14.6 2.32 204.8 10.36 1 2-193 122181 02 03 29.3 +27 38 44 02 03 28.8 +27 39 00 16919 100 14 1.35 0.07 13.9 2.17 238.0 10.26 1 2-194 122791 02 03 30.4 +26 41 51 02 03 28.8 +26 41 50 4951 71 7 0.54 0.05 7.1 2.01 68.1 8.77 1 * 2-194: possible lsb o.c. close HI coords, but larger galaxy 1.24 arcmin away (2032651+264259) 2-195 120005 02 03 40.2 +26 16 38 02 03 41.0 +26 16 36 4996 225 22 0.92 0.07 7.1 1.94 68.8 9.01 1 2-196 122792 02 03 59.4 +26 47 49 02 04 01.0 +26 48 04 14679 182 0 0.85 0.08 7.0 2.03 206.0 9.93 1 2-197 1565 02 04 32.4 +27 55 33 02 04 32.0 +27 55 31 4698 188 6 4.09 0.08 30.9 2.15 64.4 9.60 1 2-198 122183 02 05 33.8 +27 27 40 02 05 33.3 +27 27 55 12052 332 32 1.00 0.09 6.4 1.91 168.5 9.83 2 2-199 122185 02 05 59.4 +27 21 33 02 06 00.4 +27 21 31 4937 188 13 1.46 0.07 11.5 2.06 67.9 9.20 1 2-200 122793 02 06 12.7 +27 51 27 02 06 11.2 +27 51 41 7412 195 4 1.01 0.07 8.1 2.00 102.2 9.40 1 2-201 1595 02 06 26.4 +27 02 17 02 06 27.3 +27 01 59 4965 268 6 4.08 0.09 27.0 2.06 68.3 9.65 1 2-202 1638 02 08 56.3 +26 02 16 02 08 56.9 +26 02 08 4853 214 3 1.41 0.07 11.4 1.89 66.7 9.17 1 2-203 120055 02 09 01.7 +27 32 00 02 09 02.4 +27 32 10 9860 123 5 1.97 0.06 19.2 2.07 137.2 9.94 1 2-204 122186 02 09 15.7 +26 45 28 02 09 18.5 +26 45 28 12736 339 12 1.63 0.10 9.6 2.06 178.3 10.09 1 2-205 122187 02 09 55.7 +27 32 25 02 09 56.3 +27 32 34 4918 90 8 0.87 0.06 9.7 2.12 67.6 8.97 1 2-206 122794 02 11 55.2 +26 07 35 02 11 54.8 +26 07 34 4886 119 5 0.88 0.06 8.9 2.01 67.1 8.97 1 2-207 122188 02 13 10.7 +27 47 22 02 13 07.3 +27 46 49 13130 131 4 1.01 0.07 8.6 2.29 184.0 9.91 1 * 2-207: possible alternative opt.id with 021311.0+274639, very lsb system 2-208 122795 02 13 20.0 +27 51 14 02 13 17.7 +27 50 59 13180 85 3 0.67 0.06 7.2 2.27 184.7 9.73 1 * 2-208: parameters uncertain, signal possibly blended with AGC122188(021307.3+274649) 2-209 122189 02 13 31.4 +26 30 32 02 13 31.2 +26 30 49 14435 304 17 2.10 0.09 13.7 1.97 202.6 10.31 1 2-210 1718 02 14 03.2 +27 53 03 02 14 03.6 +27 52 36 592 97 10 4.84 0.07 54.9 1.99 8.4 7.91 1 2-211 122190 02 15 07.5 +26 23 18 02 15 08.1 +26 23 13 4988 196 18 1.22 0.07 10.2 1.91 68.6 9.13 1 2-212 122191 02 16 38.3 +26 08 49 02 16 39.7 +26 08 16 11332 234 15 0.98 0.08 7.4 1.93 158.3 9.76 2 2-213 122796 02 19 54.7 +26 13 03 02 19 51.7 +26 13 38 9712 216 14 1.01 0.09 7.0 2.21 135.3 9.64 1 2-214 122193 02 21 00.1 +27 02 04 02 21 01.1 +27 02 04 10804 306 26 1.78 0.09 11.3 2.02 150.9 9.98 1 2-215 122192 02 21 04.0 +27 45 49 02 21 03.4 +27 45 26 9533 170 10 2.44 0.07 19.9 2.10 132.7 10.01 1 2-216 122814 02 22 06.8 +26 04 34 -126 27 1 0.86 0.04 14.2 2.60 9 * 2-216: HVC; compact cloud but close to a larger, extended feature (AGC122816, another HVC from this catalog) 2-217 122195 02 22 27.1 +26 25 58 02 22 26.1 +26 26 10 11132 353 2 2.34 0.10 12.6 2.22 155.6 10.13 1 2-218 122799 02 22 32.1 +27 15 10 02 22 33.3 +27 14 40 9687 147 5 1.12 0.06 10.6 1.93 135.0 9.68 1 2-219 122815 02 22 49.5 +27 33 25 -129 26 1 4.30 0.09 34.6 5.36 9 * 2-219: HVC; compact cloud but close to a larger, extended feature (AGC122816, another HVC from this catalog) 2-220 120201 02 23 32.3 +27 19 24 02 23 31.3 +27 19 24 10684 235 0 0.89 0.08 6.3 2.06 149.2 9.67 2 2-221 1844 02 23 39.1 +27 09 28 02 23 39.4 +27 09 32 10646 173 6 1.91 0.08 15.3 2.13 148.7 10.00 1 2-222 122800 02 23 50.9 +26 29 48 02 23 50.7 +26 29 38 5458 124 13 0.68 0.06 6.9 1.99 75.5 8.96 1 2-223 122196 02 23 51.3 +26 22 00 02 23 47.6 +26 22 07 9563 212 30 1.00 0.08 7.8 1.98 133.2 9.62 1 2-224 1848 02 23 54.7 +27 29 22 02 23 55.5 +27 29 32 10707 435 12 3.13 0.09 17.9 1.80 149.5 10.22 1 2-225 1850 02 23 58.7 +27 07 05 02 23 58.5 +27 07 00 5467 99 4 1.11 0.05 13.1 1.90 75.6 9.18 1 2-226 122801 02 24 14.6 +27 54 57 02 24 13.1 +27 55 09 10493 56 11 0.64 0.06 8.0 2.36 146.5 9.51 1 2-227 121408 02 24 21.6 +27 14 25 02 24 23.5 +27 14 05 9679 292 29 0.78 0.09 5.0 2.05 134.9 9.52 2 2-228 122816 02 24 44.1 +26 41 19 -143 26 2 11.62 0.07 116.8 4.31 9 * 2-228: HVC; extended cloud, close in frequency to Galactic HI 2-229 120218 02 24 54.0 +26 02 25 02 25 00.2 +26 03 01 10080 312 4 2.06 0.09 12.8 2.05 140.6 9.98 1 * 2-229: previous optical redshift measurement of cz=10045 km/s, but possible alternative opt.id with 022447.3+260135 2-230 122131 02 25 16.3 +27 01 58 02 25 14.8 +27 01 55 16959 415 7 1.31 0.13 6.1 2.32 238.9 10.25 2 * 2-230: possible alternative opt.id with 022518.6+270235 2-231 122802 02 25 20.3 +27 09 01 02 25 20.2 +27 09 36 5223 159 17 0.82 0.06 7.2 2.01 72.0 9.00 1 2-232 1881 02 25 34.7 +26 44 04 02 25 35.2 +26 44 36 10333 249 31 1.94 0.09 13.4 2.04 144.2 9.98 1 2-233 120234 02 25 39.5 +27 17 48 02 25 39.5 +27 17 43 8988 177 5 2.56 0.08 19.0 2.26 125.0 9.98 1 2-234 122198 02 25 43.4 +26 57 58 02 25 45.2 +26 58 24 10000 267 46 1.21 0.08 8.0 2.07 139.5 9.74 1 2-235 122803 02 25 52.2 +27 01 00 02 25 54.3 +27 00 54 16956 166 11 1.09 0.08 8.7 2.16 238.8 10.17 1 2-236 1892 02 26 11.2 +27 36 37 02 26 12.5 +27 36 10 9976 209 10 1.50 0.08 12.0 1.94 139.1 9.84 1 2-237 122804 02 26 21.8 +26 08 06 02 26 22.7 +26 08 18 10226 193 3 1.49 0.07 11.8 2.04 142.7 9.85 1 2-238 1899 02 26 26.3 +27 39 09 02 26 26.2 +27 39 13 9732 185 34 1.06 0.09 8.1 2.14 135.7 9.66 1 2-239 1902 02 26 33.5 +27 49 20 02 26 33.7 +27 49 26 9622 267 6 2.70 0.09 17.6 2.10 134.1 10.06 1 2-240 122805 02 27 02.4 +26 58 00 02 26 59.3 +26 57 51 10370 128 20 0.86 0.07 7.4 2.28 144.8 9.63 1 2-241 122199 02 27 39.4 +26 55 04 02 27 38.5 +26 54 45 10543 182 28 1.50 0.09 11.1 2.23 147.3 9.89 1 2-242 120265 02 27 41.7 +27 13 24 02 27 40.9 +27 13 15 5126 318 6 1.29 0.09 8.1 1.99 70.6 9.18 1 2-243 120266 02 27 43.7 +26 13 05 02 27 42.3 +26 13 34 9503 313 3 2.43 0.09 14.8 2.08 132.4 10.00 1 2-244 1921 02 27 46.9 +26 35 10 02 27 46.4 +26 35 20 9793 90 16 1.34 0.06 14.1 2.23 136.5 9.77 1 2-245 121307 02 27 59.2 +27 54 33 02 27 54.9 +27 54 21 10462 254 37 1.38 0.09 8.9 2.18 146.1 9.84 1 2-246 1939 02 28 16.6 +26 18 47 02 28 17.6 +26 18 44 5222 490 27 11.47 0.13 45.9 2.28 72.0 10.15 1 2-247 122401 02 28 19.8 +26 07 14 02 28 19.5 +26 07 31 1730 90 13 1.16 0.06 13.5 2.02 23.0 8.16 1 2-248 122200 02 28 49.1 +26 45 00 02 28 49.0 +26 44 50 9544 250 9 2.61 0.08 18.7 1.97 133.0 10.04 1 2-249 122806 02 28 58.5 +26 33 18 02 28 59.8 +26 32 41 9505 89 24 0.92 0.07 9.5 2.28 132.4 9.58 1 2-250 122202 02 29 01.7 +26 04 41 02 29 01.5 +26 04 48 5895 86 9 1.14 0.06 13.1 2.09 81.9 9.26 1 2-251 122203 02 29 20.8 +27 20 59 02 29 19.9 +27 21 16 1542 41 10 0.58 0.05 10.6 1.92 20.6 7.76 1 2-252 122204 02 30 22.4 +27 57 34 02 30 23.9 +27 57 35 4736 75 3 1.10 0.05 13.9 2.04 64.8 9.04 1 2-253 122206 02 31 00.2 +27 57 51 02 31 00.3 +27 57 30 1591 73 1 3.34 0.05 41.7 2.08 21.2 8.55 1 2-254 1990 02 31 01.4 +27 42 03 02 31 04.1 +27 41 58 4584 255 23 1.43 0.10 8.6 2.32 62.6 9.12 1 2-255 122207 02 31 22.1 +26 11 56 02 31 22.1 +26 11 52 2512 144 1 3.31 0.06 29.8 2.07 33.4 8.94 1 2-256 122208 02 31 22.6 +26 47 00 02 31 24.5 +26 47 17 10980 321 5 3.29 0.09 21.6 1.90 153.6 10.26 1 2-257 122210 02 31 31.9 +26 47 58 02 31 33.0 +26 47 52 4553 84 7 1.94 0.05 23.1 2.04 62.2 9.25 1 2-258 120307 02 31 36.1 +26 10 06 02 31 34.6 +26 09 58 10868 222 4 3.31 0.08 24.0 2.07 151.9 10.26 1 * 2-258: possible alternative opt.id with 023137.2+260927, but much less likely 2-259 122211 02 31 37.5 +26 32 48 02 31 36.8 +26 32 30 3691 29 1 0.75 0.03 16.4 1.89 49.8 8.64 1 2-260 122212 02 31 40.3 +27 11 12 02 31 39.4 +27 10 46 978 34 7 0.53 0.05 9.2 2.17 13.3 7.34 1 2-261 122214 02 32 33.7 +27 56 33 02 32 33.7 +27 56 27 4657 99 15 1.00 0.06 10.6 2.11 63.7 8.98 1 2-262 2026 02 33 19.2 +27 17 51 02 33 19.2 +27 18 00 5214 160 4 1.48 0.07 12.4 2.11 71.8 9.26 1 2-263 122215 02 33 28.2 +27 11 23 02 33 28.4 +27 11 41 5343 227 15 1.36 0.08 9.1 2.21 73.7 9.24 1 2-264 122217 02 33 30.5 +27 01 06 02 33 32.3 +27 01 13 1660 76 4 1.05 0.05 13.4 1.99 22.1 8.08 1 2-265 122418 02 35 01.3 +27 13 21 02 34 59.6 +27 13 21 5194 81 11 0.61 0.06 7.3 2.07 71.5 8.87 1 2-266 122419 02 37 46.2 +26 16 18 02 37 48.2 +26 16 49 10006 104 29 0.66 0.06 7.5 1.92 139.7 9.48 1 2-267 122420 02 38 50.5 +27 21 59 02 38 50.0 +27 21 56 1463 60 3 1.05 0.04 15.4 1.96 19.5 7.97 1 2-268 2134 02 38 51.7 +27 50 46 02 38 51.9 +27 50 48 4586 327 7 9.17 0.08 61.9 1.83 62.6 9.93 1 2-269 122219 02 40 55.0 +26 39 58 02 40 55.6 +26 40 05 1482 34 4 0.48 0.05 8.0 2.29 19.7 7.64 1 2-270 122220 02 41 25.0 +26 23 32 02 41 24.5 +26 23 21 10619 255 36 0.96 0.08 7.0 1.93 148.5 9.70 1 2-271 122421 02 41 32.7 +26 37 21 02 41 31.7 +26 37 45 1586 41 6 0.80 0.05 13.0 2.13 21.1 7.92 1 2-272 122221 02 44 19.0 +26 06 59 02 44 18.5 +26 06 29 10565 188 10 1.19 0.08 8.5 2.28 147.8 9.79 1 * 2-272: several possible alternative opt.id, but candidate selected on previous cz information and spatial proximity 2-273 122422 02 44 24.3 +27 39 03 02 44 23.7 +27 38 34 8082 210 32 0.90 0.09 6.2 2.26 112.4 9.43 1 2-274 122423 02 45 03.7 +26 04 18 02 45 04.6 +26 04 27 14271 329 45 1.50 0.11 8.0 2.32 200.8 10.15 1 2-275 2236 02 46 11.0 +27 02 51 02 46 11.1 +27 02 41 5731 207 7 4.12 0.09 27.7 2.31 79.4 9.79 1 2-276 122226 02 46 38.9 +27 43 35 02 46 38.9 +27 43 35 472 29 1 2.04 0.04 39.0 2.16 6.8 7.35 1 2-277 2268 02 47 54.1 +26 05 29 02 47 55.4 +26 05 40 7573 173 3 1.15 0.07 8.7 2.24 105.1 9.48 1 2-278 2272 02 48 03.9 +27 06 05 02 48 04.5 +27 06 09 5650 478 4 5.95 0.10 28.6 1.94 78.2 9.93 1 2-279 122427 02 49 36.2 +27 00 22 02 49 37.0 +27 00 20 10170 243 17 1.57 0.08 11.5 1.96 142.3 9.88 1 2-280 122428 02 49 52.3 +26 39 41 02 49 51.8 +26 39 32 7120 123 12 1.01 0.07 9.6 2.11 98.7 9.37 1 2-281 122223 02 51 24.8 +26 34 51 02 51 23.1 +26 34 58 7483 150 3 3.11 0.07 25.6 2.21 103.9 9.90 1 2-282 122224 02 51 49.8 +26 03 17 02 51 50.0 +26 03 10 10158 192 5 2.26 0.08 16.4 2.22 142.1 10.03 1 2-283 122836 02 52 14.5 +26 26 29 -135 29 3 3.83 0.08 29.7 5.17 9 2-284 122429 02 53 53.3 +26 30 32 02 53 52.7 +26 30 27 6176 254 5 1.36 0.08 9.9 1.92 85.3 9.37 1 2-285 122431 02 56 04.7 +26 43 28 02 56 04.0 +26 43 35 10542 318 72 1.70 0.09 10.2 2.09 147.7 9.94 1 2-286 121023 02 56 09.2 +27 42 11 02 56 08.1 +27 42 04 6473 222 17 2.54 0.08 19.4 1.96 89.6 9.68 1 2-287 122432 02 56 14.8 +26 27 55 02 56 12.9 +26 28 08 10587 169 17 0.81 0.07 6.7 2.07 148.3 9.62 1 2-288 122807 02 57 43.6 +26 16 24 02 57 42.0 +26 16 38 10370 221 12 1.10 0.07 8.6 1.92 145.3 9.74 1 2-289 122809 02 59 07.5 +27 10 58 02 59 05.6 +27 10 56 10842 173 21 1.05 0.07 7.9 2.24 152.0 9.76 1 * 2-289: possible alternative opt.id with 025906.9+271143, irregular lsb galaxy farther from the HI center 2-290 131358 03 00 31.4 +26 51 13 03 00 29.7 +26 50 53 10706 259 28 1.58 0.09 9.6 2.27 150.1 9.92 1 2-291 131359 03 00 43.6 +27 13 43 03 00 44.3 +27 13 24 10513 209 177 1.11 0.08 8.5 2.02 147.4 9.76 1 2-292 131360 03 02 55.0 +26 00 09 03 02 54.4 +26 00 25 10618 117 4 1.66 0.07 16.0 2.13 148.9 9.94 1 2-293 131361 03 03 05.6 +27 33 45 03 03 04.5 +27 33 46 6943 181 9 2.13 0.07 17.8 1.98 96.4 9.67 1 2-294 321218 22 00 37.5 +27 20 49 22 00 37.0 +27 20 54 12737 151 25 1.07 0.08 8.3 2.33 177.2 9.90 1 2-295 321195 22 00 40.7 +27 20 18 22 00 39.8 +27 20 20 5870 219 4 3.41 0.08 24.3 2.11 85.9 9.77 1 2-296 321196 22 00 59.4 +27 37 21 22 00 59.5 +27 36 51 3511 82 9 0.71 0.06 8.4 2.08 53.0 8.67 1 2-297 321197 22 02 38.3 +27 20 06 22 02 38.3 +27 19 35 6942 128 3 0.95 0.07 8.8 2.14 94.4 9.30 1 2-298 320013 22 04 12.8 +26 22 50 22 04 12.1 +26 22 22 6095 131 20 0.77 0.06 7.6 1.96 82.3 9.09 1 2-299 320019 22 05 09.8 +26 36 37 22 05 08.8 +26 36 25 6102 249 31 2.85 0.09 18.5 2.19 82.4 9.66 1 2-300 321198 22 06 00.5 +26 15 50 22 06 01.6 +26 15 55 11817 167 2 1.14 0.07 9.3 2.12 164.0 9.86 1 2-301 321199 22 08 05.6 +27 02 28 22 08 06.8 +27 02 21 7089 175 13 1.34 0.07 10.8 2.09 96.5 9.47 1 2-302 321201 22 11 36.1 +26 02 21 22 11 35.5 +26 02 32 12404 148 10 1.14 0.08 8.7 2.41 172.4 9.90 1 2-303 321205 22 14 57.9 +26 57 06 22 14 55.9 +26 57 28 4367 105 17 1.06 0.06 10.7 2.16 64.6 9.02 1 2-304 320116 22 16 12.8 +27 54 18 22 16 11.6 +27 54 21 7088 286 5 4.16 0.09 27.6 1.99 96.5 9.96 1 2-305 320136 22 17 42.9 +27 37 49 22 17 44.7 +27 37 26 6553 296 26 0.89 0.09 5.7 2.05 88.8 9.22 2 2-306 321217 22 18 20.4 +27 52 11 22 18 20.4 +27 52 22 3572 148 3 2.04 0.06 19.0 1.97 53.4 9.14 1 2-307 321206 22 18 50.6 +26 41 51 22 18 51.2 +26 42 08 6630 62 3 0.67 0.05 9.3 2.03 89.9 9.11 1 2-308 321207 22 18 52.4 +27 37 55 22 18 51.5 +27 37 35 3584 96 0 1.04 0.06 10.6 2.24 53.5 8.85 1 2-309 321290 22 19 10.1 +27 03 51 -431 48 4 0.52 0.06 5.4 3.10 9 * 2-309: HVC; end of the extension of a cloud located 1 degree away (AGC321292, another HVC from this catalog) 2-310 321208 22 19 50.6 +26 24 02 22 19 50.6 +26 23 56 12422 25 3 0.52 0.04 11.0 2.07 172.6 9.56 1 2-311 321291 22 21 07.8 +26 42 32 -412 29 1 1.57 0.08 13.5 4.82 9 * 2-311: HVC; part of the extension of a cloud (AGC321292, another HVC from this catalog) that extends over 1 degree 2-312 321209 22 21 20.9 +27 50 27 22 21 21.0 +27 50 33 12706 303 26 1.37 0.11 8.0 2.20 176.7 10.00 1 * 2-312: possible alternative opt.id with 222120.9+274943, edge-on disc 2-313 321211 22 23 21.0 +26 25 40 22 23 21.6 +26 25 28 12399 360 38 2.67 0.11 14.8 2.12 172.3 10.27 1 2-314 321293 22 25 36.6 +26 52 52 -470 36 2 0.63 0.05 8.5 2.73 9 * 2-314: compact HVC; separated in velocity by about 100 km/s from other nearby clouds 2-315 321212 22 28 07.1 +26 12 56 22 28 07.5 +26 13 07 10090 159 3 1.08 0.07 9.1 2.11 139.2 9.69 1 2-316 321213 22 28 37.3 +26 37 48 22 28 37.2 +26 37 47 12345 243 6 2.27 0.08 16.2 2.01 171.5 10.20 1 2-317 321214 22 29 17.6 +27 48 10 22 29 15.7 +27 48 17 12091 227 38 0.99 0.09 6.6 2.23 167.9 9.82 1 2-318 321215 22 29 32.8 +26 58 20 22 29 31.6 +26 58 17 4231 70 7 0.79 0.05 10.3 2.06 62.3 8.86 1 2-319 321294 22 31 30.8 +26 37 14 -391 37 2 0.66 0.08 5.9 4.11 9 * 2-319: HVC; in the vicinity of other clouds 2-320 321295 22 34 27.8 +27 03 46 -386 29 4 0.53 0.05 7.7 2.81 9 * 2-320: HVC; in the vicinity of other clouds 2-321 321282 22 34 45.9 +27 06 19 22 34 43.9 +27 06 26 13214 28 3 0.55 0.04 10.6 2.17 183.9 9.64 1 2-322 321283 22 36 25.3 +26 45 00 22 36 26.0 +26 44 57 10102 240 6 1.50 0.08 11.3 1.91 139.4 9.84 1 2-323 321296 22 39 42.9 +27 33 22 -441 24 6 0.47 0.05 9.0 2.38 9 * 2-323: HVC; in the vicinity of other clouds 2-324 321297 22 40 23.4 +26 09 49 -421 36 2 1.42 0.09 10.1 5.17 9 * 2-324: HVC; in the vicinity of other clouds 2-325 321286 22 42 06.6 +27 46 31 22 42 07.3 +27 46 11 6964 155 4 1.22 0.07 9.9 2.20 94.6 9.41 1 2-326 321287 22 42 34.8 +27 45 51 22 42 35.0 +27 45 51 11954 309 8 1.16 0.09 7.1 2.07 165.9 9.88 1 2-327 12193 22 48 43.7 +27 35 37 22 48 44.2 +27 35 00 9599 333 4 9.26 0.09 55.3 2.05 132.2 10.58 1 * 2-327: HI signal is most likely a blend between AGC12191(224840.9+273638) and AGC12193(224844.2+273500). Opt.id made with 12193 which is closer to the HI coordinates 2-328 12194 22 48 49.9 +27 57 34 22 48 50.8 +27 57 45 10025 367 10 2.31 0.09 14.0 1.92 138.3 10.02 1 2-329 12198 22 49 09.1 +27 52 02 22 49 10.8 +27 51 54 9987 422 8 1.75 0.10 9.2 2.01 137.8 9.89 1 2-330 321298 22 50 24.0 +26 06 23 -401 30 1 0.59 0.06 6.2 3.87 9 * 2-330: HVC; faint, in the vicinity of other clouds 2-331 321299 22 51 18.9 +26 24 34 -417 34 3 0.65 0.05 7.8 3.18 9 * 2-331: HVC; faint, in the vicinity of other clouds 2-332 321289 22 53 19.8 +26 46 18 22 53 21.6 +26 45 53 10054 247 23 1.42 0.08 9.8 2.05 138.7 9.81 1 2-333 321310 22 54 38.9 +27 13 46 -412 30 9 0.88 0.08 8.4 4.16 9 * 2-333: HVC; faint, in the vicinity of other clouds 2-334 321226 22 55 43.4 +26 18 28 22 55 44.8 +26 18 10 4372 117 25 1.00 0.06 10.4 1.98 63.6 8.98 1 2-335 320926 22 55 58.1 +26 10 06 22 55 58.5 +26 10 07 2648 58 1 2.08 0.05 30.2 2.01 39.2 8.88 1 2-336 320862 22 56 50.5 +26 50 28 22 56 50.7 +26 50 36 7494 205 4 2.59 0.07 20.7 1.95 102.1 9.80 1 2-337 320466 22 57 20.9 +27 59 02 22 57 21.5 +27 58 50 2945 107 1 2.74 0.05 29.4 2.02 43.3 9.08 1 2-338 320467 22 57 27.6 +26 06 06 22 57 28.2 +26 06 26 7103 286 7 1.08 0.11 6.2 2.32 96.5 9.38 2 2-339 321227 22 57 32.8 +26 20 17 22 57 32.0 +26 20 10 7078 213 2 1.40 0.08 9.7 2.21 96.1 9.48 1 2-340 321228 22 58 25.1 +26 01 49 22 58 23.2 +26 01 42 7492 104 13 0.71 0.06 8.0 1.95 102.1 9.24 1 2-341 321229 22 58 59.9 +27 21 50 22 58 59.4 +27 21 53 9681 193 11 0.89 0.08 7.1 2.01 133.4 9.57 1 2-342 320806 22 59 02.1 +26 23 15 22 58 58.3 +26 23 07 7627 211 10 1.61 0.08 11.5 2.16 104.0 9.61 1 2-343 321230 22 59 47.8 +27 33 13 22 59 46.2 +27 33 19 9559 355 63 2.28 0.11 11.9 2.27 131.6 9.97 1 2-344 12291 22 59 47.9 +26 18 06 22 59 48.3 +26 18 07 7761 312 4 4.30 0.09 25.4 2.14 105.9 10.06 1 2-345 12293 22 59 51.1 +26 01 59 22 59 51.6 +26 01 58 9964 59 10 1.95 0.06 29.1 1.96 137.4 9.94 1 2-346 320497 23 00 10.8 +26 05 14 23 00 11.1 +26 05 46 6839 108 3 1.68 0.06 17.6 2.05 92.7 9.53 1 * 2-346: possible alternative opt.id with small lsb galaxy closer to HI center at 230012.6+260512 2-347 12303 23 00 49.3 +26 44 36 23 00 49.1 +26 44 26 7946 269 4 4.61 0.09 31.0 2.03 108.6 10.11 1 2-348 12319 23 02 04.4 +27 03 06 23 02 03.4 +27 03 08 7508 415 6 7.04 0.11 34.4 2.20 102.3 10.24 1 2-349 12327 23 02 53.5 +26 00 51 23 02 53.7 +26 00 52 12820 396 8 2.89 0.11 15.6 2.09 178.2 10.34 1 2-350 332905 23 04 09.8 +27 08 02 23 04 11.3 +27 07 14 7613 178 19 1.09 0.08 8.8 2.08 103.8 9.44 1 2-351 12340 23 04 33.7 +27 09 17 23 04 33.8 +27 09 21 1056 112 1 6.99 0.07 63.3 2.33 16.5 8.65 1 2-352 12352 23 05 42.0 +27 40 13 23 05 40.4 +27 39 54 7456 450 38 1.81 0.11 8.3 2.15 101.6 9.64 1 2-353 332908 23 05 44.7 +27 12 47 23 05 43.4 +27 12 46 7406 92 6 0.74 0.07 8.0 2.14 100.9 9.25 1 2-354 332909 23 05 46.1 +26 43 51 23 05 46.2 +26 43 32 7335 185 2 1.51 0.07 12.0 2.07 99.8 9.55 1 2-355 330051 23 06 20.8 +27 53 00 23 06 19.9 +27 53 26 6902 78 2 0.50 0.06 5.9 2.15 93.7 9.02 2 2-356 330065 23 07 28.6 +27 40 53 23 07 30.3 +27 41 00 7048 385 80 1.10 0.11 5.6 2.22 95.8 9.38 2 2-357 330070 23 08 18.1 +27 43 01 23 08 17.9 +27 43 02 2883 83 2 3.89 0.05 49.1 1.93 42.2 9.21 1 2-358 332911 23 08 54.6 +27 36 34 23 08 54.5 +27 36 29 7256 196 3 1.57 0.08 11.9 2.11 98.7 9.56 1 2-359 333203 23 10 15.2 +27 47 54 23 10 13.1 +27 47 40 9187 144 8 0.69 0.06 7.3 1.73 126.3 9.41 1 2-360 332912 23 11 58.6 +27 17 24 23 12 01.0 +27 17 41 794 27 1 0.52 0.04 10.9 2.03 12.7 7.30 1 2-361 332913 23 12 57.9 +27 20 46 23 12 57.2 +27 20 52 7200 124 12 0.70 0.06 6.9 2.02 97.9 9.20 1 2-362 330168 23 16 00.8 +27 27 06 23 15 59.6 +27 27 13 7339 134 4 2.53 0.06 24.5 1.98 99.9 9.78 1 2-363 332299 23 16 09.8 +26 00 49 23 16 10.2 +26 00 35 7522 156 45 0.61 0.06 5.4 2.02 102.5 9.18 2 2-364 332333 23 17 14.6 +27 59 14 7061 170 1 1.48 0.06 13.4 1.88 95.9 9.51 1 * 2-364: opt.id ambiguous; possible counterparts at 231717.3+275839, 231710.2+275858 2-365 12499 23 19 08.7 +26 09 07 23 19 07.0 +26 09 09 5564 183 4 1.58 0.07 12.9 2.03 79.9 9.38 1 2-366 330226 23 19 14.1 +26 03 09 23 19 14.4 +26 03 20 6259 207 4 0.97 0.08 7.7 1.96 84.4 9.21 1 2-367 332915 23 19 25.9 +26 06 36 23 19 27.8 +26 06 30 3564 187 44 1.20 0.08 9.0 2.19 51.5 8.88 1 2-368 12514 23 19 56.7 +26 00 29 23 19 55.3 +26 00 41 5867 245 3 2.18 0.07 17.0 1.84 84.2 9.56 1 2-369 330244 23 20 05.1 +26 13 10 23 20 03.0 +26 12 57 7997 201 23 0.86 0.08 6.6 2.08 109.3 9.38 1 2-370 330247 23 20 05.4 +26 01 31 23 20 09.9 +26 01 23 6038 246 2 1.72 0.08 12.4 1.98 81.3 9.43 1 * 2-370: parameters uncertain, HI signal partly blended with AGC12514(231955.3+260041) 2-371 332918 23 20 20.8 +27 51 07 23 20 23.7 +27 51 49 3625 117 0 0.65 0.05 7.4 1.80 52.3 8.62 1 2-372 12527 23 20 22.7 +27 18 58 23 20 22.6 +27 18 55 4272 266 19 2.71 0.09 17.2 2.15 61.5 9.38 1 2-373 330263 23 21 04.7 +26 25 17 23 21 03.8 +26 25 11 5826 132 7 1.87 0.06 18.3 1.98 83.5 9.49 1 2-374 332920 23 21 12.7 +26 05 29 23 21 12.3 +26 05 33 4299 115 2 2.29 0.06 21.9 2.17 61.9 9.32 1 2-375 331622 23 21 29.2 +26 28 22 23 21 27.9 +26 28 41 5899 203 2 2.34 0.08 18.2 2.01 84.6 9.60 1 2-376 332236 23 21 34.5 +26 05 55 23 21 37.1 +26 06 22 4315 28 1 0.38 0.04 7.3 2.13 62.1 8.54 1 2-377 12543 23 21 37.7 +27 05 28 23 21 33.5 +27 07 05 5969 298 9 4.75 0.09 29.8 2.06 85.6 9.91 1 * 2-377: parameters uncertain, signal partly blended with AGC12546(232141.2+270512) 2-378 12546 23 21 38.4 +27 05 23 23 21 41.2 +27 05 12 6055 340 6 3.77 0.09 22.3 2.05 81.6 9.77 1 * 2-378: parameters uncertain, signal partly blended with AGC12543(232133.5+270705) 2-379 332921 23 21 40.1 +27 51 52 23 21 40.7 +27 51 29 3650 102 6 0.57 0.05 6.5 1.93 52.6 8.57 1 * 2-379: possible alternative opt.id with 232136.3+275216.8 but farther from HI center 2-380 12545 23 21 41.6 +27 04 05 23 21 41.9 +27 04 15 5754 236 4 4.06 0.08 27.2 2.17 82.5 9.81 1 * 2-380: parameters uncertain, signal partly blended with AGC12546(232141.2+270512) 2-381 330281 23 21 42.0 +27 40 01 23 21 42.0 +27 39 46 5925 62 12 1.11 0.05 14.2 2.20 85.0 9.28 1 2-382 330287 23 22 05.5 +27 31 04 23 22 06.0 +27 31 19 2922 158 8 1.95 0.12 10.7 3.23 42.3 8.92 1 * 2-382: poor baseline, galaxy very near 1.3 Jy continuum source 2-383 330310 23 22 51.5 +26 16 28 23 22 51.2 +26 16 37 12648 230 20 0.96 0.08 6.6 2.16 175.7 9.84 2 2-384 332936 23 23 52.0 +27 53 45 23 23 54.2 +27 53 23 6245 152 1 1.07 0.07 8.9 2.18 84.3 9.25 1 2-385 332924 23 24 33.0 +27 51 28 23 24 32.8 +27 51 11 6757 129 3 1.36 0.07 13.3 2.00 91.6 9.43 1 2-386 332308 23 24 36.4 +27 56 15 23 24 37.7 +27 56 28 5857 166 16 0.79 0.06 6.8 2.04 83.9 9.12 1 2-387 12587 23 24 50.5 +26 38 35 23 24 49.9 +26 38 45 12790 357 7 1.22 0.11 6.7 2.16 177.8 9.96 1 2-388 332926 23 25 58.0 +27 01 58 23 25 57.9 +27 02 28 6111 137 8 1.85 0.07 17.3 2.04 82.4 9.47 1 2-389 332927 23 26 27.2 +26 49 00 23 26 26.8 +26 49 18 7599 141 1 0.90 0.07 7.5 2.24 103.6 9.36 1 2-390 332929 23 26 33.6 +26 55 43 23 26 31.3 +26 56 15 5818 76 12 0.96 0.07 11.0 2.22 83.3 9.20 1 2-391 330451 23 26 47.3 +26 36 11 23 26 46.8 +26 36 11 5713 230 3 3.66 0.08 24.7 2.18 81.8 9.76 1 2-392 332930 23 27 05.1 +26 00 29 23 27 04.2 +26 00 06 13104 69 4 0.53 0.06 7.0 2.03 182.2 9.62 1 2-393 332919 23 27 43.0 +27 13 21 23 27 42.1 +27 13 26 5079 130 6 0.90 0.06 8.3 2.13 72.8 9.05 1 2-394 332914 23 27 53.7 +26 23 23 23 27 54.0 +26 23 33 7980 160 10 1.54 0.07 13.4 2.04 109.0 9.64 1 2-395 332916 23 27 59.5 +26 09 15 23 28 00.2 +26 09 42 8553 59 2 0.70 0.04 10.3 1.97 117.2 9.36 1 2-396 332917 23 28 40.8 +27 44 31 23 28 40.4 +27 44 17 5673 131 13 1.01 0.05 10.7 1.84 81.2 9.20 1 2-397 332940 23 28 41.4 +27 17 48 23 28 41.0 +27 18 14 5787 139 7 1.64 0.06 14.8 2.10 82.8 9.42 1 2-398 12626 23 29 15.7 +26 22 41 23 29 15.2 +26 22 45 8022 444 5 6.85 0.10 36.2 1.90 109.6 10.29 1 2-399 333204 23 29 20.5 +26 18 15 23 29 20.2 +26 17 41 8099 118 15 1.44 0.06 14.4 2.04 110.7 9.62 1 * 2-399: parameters uncertain, signal blended with AGC12626(232915.2+262245). HI seen to extend from AGC12626 to AGC333204(232920.2+261741), most likely an interacting pair. 2-400 332941 23 29 53.8 +27 23 09 23 29 53.4 +27 22 46 7142 219 22 1.14 0.08 8.0 2.16 97.1 9.40 1 2-401 12631 23 30 00.6 +27 05 05 23 30 01.2 +27 05 11 9184 446 4 3.66 0.11 17.4 2.10 126.3 10.14 1 2-402 12636 23 30 19.9 +27 08 06 23 30 19.2 +27 08 00 7335 231 7 2.78 0.08 18.9 2.17 99.8 9.82 1 2-403 331192 23 30 28.7 +26 08 41 23 30 30.0 +26 07 56 8045 219 11 1.20 0.08 8.7 2.07 110.0 9.53 1 2-404 332961 23 30 43.5 +26 21 58 23 30 43.8 +26 22 48 7865 187 13 0.92 0.07 7.0 2.15 107.4 9.40 1 * 2-404: possible alternative opt.id with 233039.8+262145 2-405 332942 23 30 44.8 +26 13 58 23 30 44.9 +26 14 11 7885 136 7 2.26 0.07 20.9 2.07 107.7 9.79 1 2-406 330514 23 31 46.0 +27 18 58 23 31 42.6 +27 19 09 12702 417 12 1.25 0.12 5.7 2.34 176.5 9.96 2 2-407 332943 23 31 57.3 +26 18 56 23 31 57.7 +26 19 40 9397 170 0 0.78 0.07 6.0 2.24 129.3 9.49 1 2-408 332944 23 31 59.0 +26 48 54 23 31 55.6 +26 49 12 14796 274 6 1.29 0.10 7.7 2.28 206.4 10.11 1 2-409 330532 23 33 13.1 +26 52 28 23 33 12.8 +26 52 16 3691 132 1 6.51 0.07 58.2 2.17 52.9 9.63 1 2-410 332945 23 33 36.6 +26 14 05 23 33 37.7 +26 14 26 3687 72 3 0.69 0.05 9.3 1.97 52.8 8.66 1 2-411 332946 23 33 37.8 +27 27 41 23 33 37.2 +27 27 12 7576 74 8 0.68 0.06 8.7 2.02 103.3 9.23 1 2-412 331201 23 33 42.0 +27 19 00 23 33 40.4 +27 18 59 9169 217 4 1.32 0.08 9.5 2.11 126.1 9.69 1 2-413 12678 23 34 46.5 +26 18 22 23 34 48.6 +26 18 38 9092 237 4 1.20 0.09 8.2 2.14 124.9 9.65 1 * 2-413: parameters uncertain, signal blending with strong rfi 2-414 333226 23 35 05.4 +27 09 48 -441 25 1 2.31 0.08 17.5 5.84 9 * 2-414: HVC; one of two knots in a small clumpy cloud 2-415 331218 23 35 18.3 +26 17 54 23 35 18.0 +26 17 44 8034 67 2 1.10 0.05 15.3 1.98 109.8 9.50 1 2-416 331221 23 35 40.1 +26 39 03 23 35 41.5 +26 39 02 7893 149 0 0.88 0.06 8.4 1.91 107.8 9.38 1 2-417 333227 23 35 43.5 +26 54 46 -439 21 1 0.74 0.04 12.4 2.87 9 * 2-417: HVC; one of two knots in a small clumpy cloud 2-418 331225 23 35 53.9 +26 09 26 23 35 50.9 +26 08 34 8056 288 52 1.07 0.09 6.7 2.09 110.1 9.49 2 2-419 332947 23 36 14.0 +26 21 50 23 36 13.3 +26 21 41 11820 177 13 1.02 0.07 8.1 2.12 163.9 9.81 1 2-420 331230 23 36 19.8 +26 22 10 23 36 23.9 +26 22 11 8037 243 1 0.82 0.08 5.7 2.08 109.9 9.37 2 2-421 12701 23 36 25.4 +27 56 09 23 36 25.7 +27 56 08 8917 200 27 2.16 0.07 17.4 1.95 122.5 9.88 1 * 2-421: parameters uncertain, signal blending with strong rfi 2-422 330584 23 37 05.7 +27 03 28 23 37 01.9 +27 03 40 10324 174 64 0.71 0.08 5.3 2.26 142.6 9.53 2 2-423 332948 23 37 06.7 +26 25 44 23 37 07.7 +26 26 10 9761 158 44 0.98 0.09 7.0 2.50 134.5 9.62 1 * 2-423: possible alternative opt.id with 233705.4+262541, lower surface brightness but closer from HI detection center 2-424 332963 23 38 02.3 +26 48 58 23 38 02.5 +26 49 36 7979 120 8 0.97 0.07 8.7 2.27 109.1 9.43 1 * 2-424: possible alternative opt.id with 233759.6+264810 2-425 332949 23 38 04.9 +27 50 21 23 38 05.1 +27 50 14 12773 202 25 1.91 0.09 13.7 2.18 177.6 10.15 1 2-426 330636 23 38 11.3 +27 12 28 23 38 09.9 +27 12 08 7961 123 14 1.78 0.07 16.3 2.20 108.8 9.70 1 2-427 330661 23 38 33.1 +26 35 35 23 38 30.1 +26 35 51 9389 162 11 1.48 0.11 8.2 3.18 129.2 9.77 1 2-428 331463 23 38 58.6 +26 12 19 23 38 56.4 +26 12 05 11476 269 43 1.30 0.10 7.8 2.26 159.0 9.89 2 2-429 330714 23 39 07.4 +26 34 48 23 39 05.9 +26 34 49 7920 128 32 0.72 0.09 4.9 2.91 108.2 9.30 2 2-430 330718 23 39 07.4 +26 41 10 23 39 09.8 +26 41 35 8163 210 12 1.87 0.10 11.0 2.61 111.7 9.74 1 2-431 333228 23 39 11.1 +27 32 51 -144 24 1 1.01 0.06 11.2 4.05 9 * 2-431: HVC; lower velocity than other clouds, merging with Galactic emission 2-432 12721 23 39 13.8 +27 06 50 23 39 11.9 +27 06 55 7602 401 2 5.99 0.10 33.7 1.98 103.7 10.18 1 2-433 330751 23 40 08.4 +26 54 15 23 40 08.6 +26 54 01 11101 150 23 0.85 0.08 7.0 2.21 153.7 9.68 1 2-434 330761 23 40 36.6 +27 11 15 23 40 42.4 +27 10 39 10173 146 61 0.90 0.08 6.8 2.44 140.4 9.62 2 2-435 12732 23 40 40.1 +26 13 49 23 40 39.8 +26 14 10 747 118 1 59.94 0.08 467.0 2.63 11.6 9.28 1 2-436 331266 23 40 52.4 +27 27 04 23 40 51.7 +27 27 13 4471 98 8 1.91 0.06 19.3 2.22 63.8 9.26 1 2-437 332951 23 42 39.0 +27 49 51 23 42 36.8 +27 49 37 2751 110 4 6.18 0.08 59.6 2.21 39.3 9.35 1 * 2-437: possible alternative opt.id with AGC330782(234244.7+275056), but 1.9arcmin away from HI center. Surprisingly bright HI given the morphology of the galaxy. 2-438 330779 23 42 39.5 +27 05 32 23 42 38.3 +27 05 30 7483 285 2 1.35 0.09 8.4 2.12 102.0 9.52 1 2-439 330781 23 42 40.4 +27 07 04 23 42 41.0 +27 07 30 7716 267 9 1.87 0.09 12.4 2.06 105.3 9.69 1 2-440 12746 23 42 46.4 +27 17 45 23 42 46.7 +27 17 49 7441 460 16 5.42 0.11 25.8 2.04 101.4 10.12 1 2-441 332953 23 42 57.9 +27 40 42 23 42 58.4 +27 40 26 7866 112 1 0.91 0.06 9.2 2.09 107.5 9.39 1 2-442 331305 23 43 23.3 +26 54 58 23 43 24.3 +26 54 57 8189 296 11 2.06 0.09 12.5 2.14 112.1 9.79 1 * 2-442: possible alternative opt.id with AGC331304(234323.0+265517) 2-443 332954 23 43 50.4 +27 08 16 23 43 49.7 +27 08 16 7532 95 12 0.75 0.05 8.1 2.11 102.7 9.27 1 * 2-443: very rich field, opt.id ambiguous 2-444 12754 23 43 54.1 +26 04 29 23 43 54.5 +26 04 31 750 191 0 40.19 0.07 291.5 2.23 11.6 9.11 1 2-445 332957 23 43 56.7 +27 06 28 23 43 55.3 +27 06 21 7801 28 2 0.60 0.04 12.3 2.05 106.5 9.21 1 2-446 333202 23 44 00.5 +27 09 52 23 44 00.0 +27 09 12 6745 84 10 0.64 0.06 7.3 2.13 91.5 9.10 1 2-447 331319 23 44 50.5 +26 48 58 23 44 49.7 +26 48 52 7775 180 20 1.69 0.07 12.9 2.17 106.2 9.65 1 2-448 331322 23 45 18.7 +27 28 29 23 45 18.3 +27 28 20 9206 275 10 1.93 0.09 12.5 2.08 126.6 9.86 1 2-449 12772 23 45 35.1 +27 21 13 23 45 32.2 +27 21 37 7690 539 29 1.40 0.11 5.8 2.02 105.0 9.56 2 2-450 333229 23 45 44.5 +26 22 11 -409 29 1 0.63 0.05 9.0 2.89 9 * 2-450: HVC; faint cloud, near brighter object AGC333230 2-451 330888 23 45 47.5 +27 35 51 23 45 47.4 +27 35 51 8974 198 21 1.69 0.07 13.8 1.95 123.3 9.78 1 * 2-451: parameters uncertain, signal blending with strong rfi 2-452 333207 23 46 52.8 +27 19 43 23 46 53.8 +27 19 18 9387 340 2 1.30 0.09 7.8 2.02 129.2 9.71 1 * 2-452: possible alternative opt.id with 234657.7+272012 but farther from HI center 2-453 331415 23 46 52.9 +27 37 34 23 46 51.7 +27 37 18 8007 116 23 0.95 0.05 10.1 1.95 109.5 9.43 1 2-454 331333 23 47 03.0 +27 16 58 23 47 01.3 +27 16 24 8965 192 32 1.66 0.07 13.4 1.99 123.2 9.77 1 * 2-454: parameters uncertain, signal blending with strong rfi 2-455 331344 23 47 47.1 +26 09 42 23 47 47.5 +26 09 04 11474 165 46 1.10 0.07 9.0 2.13 159.0 9.82 1 2-456 330924 23 47 48.2 +27 40 58 23 47 46.1 +27 40 53 6822 237 5 1.32 0.08 9.1 2.11 92.6 9.43 1 2-457 330925 23 48 01.7 +27 37 53 23 48 01.7 +27 37 24 8308 377 0 2.09 0.09 12.2 1.97 113.8 9.81 1 2-458 333230 23 48 04.4 +26 54 09 -435 23 1 1.85 0.05 23.1 3.67 9 * 2-458: HVC; patchy, fairly bright cloud, with two fainter clouds nearby 2-459 331345 23 48 04.4 +27 33 03 23 48 01.2 +27 32 58 8430 229 31 1.54 0.08 10.1 2.24 115.5 9.69 1 * 2-459: parameters possibly uncertain, signal blending with strong rfi 2-460 330928 23 48 25.7 +27 56 45 23 48 24.2 +27 56 58 6850 277 12 1.70 0.09 11.4 2.01 93.0 9.54 1 2-461 12791 23 48 51.0 +26 13 05 23 48 49.3 +26 13 14 789 90 2 5.41 0.05 60.1 2.11 12.1 8.27 1 2-462 12792 23 49 01.0 +26 47 32 23 49 01.5 +26 47 17 11514 422 4 3.15 0.10 16.6 2.00 159.6 10.28 1 2-463 333211 23 49 12.8 +27 16 45 23 49 11.4 +27 16 05 8416 170 21 0.99 0.07 7.7 2.18 115.3 9.49 1 2-464 332317 23 49 37.5 +27 56 03 23 49 37.5 +27 55 55 6828 235 3 2.26 0.08 16.1 2.05 92.7 9.66 1 2-465 331353 23 49 52.6 +26 20 22 23 49 51.7 +26 20 19 7296 209 1 2.76 0.08 19.4 2.19 99.3 9.81 1 2-466 330953 23 50 45.2 +27 17 16 23 50 47.4 +27 17 16 7995 98 6 1.68 0.07 17.9 2.12 109.3 9.68 1 * 2-466: possible alternative opt.id with 235044.5+271642, a very lsb system 2-467 333214 23 51 40.6 +27 28 09 23 51 37.9 +27 28 10 2836 20 2 0.50 0.03 13.1 1.88 40.3 8.28 1 2-468 330980 23 51 57.5 +27 19 34 23 51 58.9 +27 20 15 8155 261 33 1.12 0.08 7.4 2.08 111.6 9.52 1 2-469 333216 23 52 23.4 +27 44 43 23 52 22.9 +27 44 19 7255 110 5 0.87 0.05 10.3 1.79 98.8 9.30 1 2-470 331372 23 52 28.1 +27 08 28 23 52 27.8 +27 08 39 16809 182 10 1.00 0.08 7.4 2.24 235.2 10.12 1 * 2-470: possible alternative opt.id with 235227.1+270901 2-471 333217 23 52 49.5 +27 18 32 23 52 50.0 +27 18 24 7173 158 5 0.95 0.06 8.7 1.94 97.6 9.33 1 2-472 333218 23 52 49.3 +27 30 09 23 52 48.6 +27 30 07 5233 168 2 2.71 0.06 23.5 1.98 74.4 9.55 1 2-473 331375 23 53 00.6 +26 29 24 23 52 59.6 +26 29 40 8231 277 5 0.87 0.08 5.9 1.99 112.7 9.42 2 2-474 331377 23 53 10.1 +26 40 00 23 53 11.3 +26 39 54 7449 165 12 1.66 0.07 14.5 2.00 101.5 9.61 1 2-475 331382 23 54 03.9 +26 26 14 23 54 04.5 +26 26 49 7443 224 2 1.56 0.08 10.9 2.14 101.4 9.58 1 2-476 331383 23 54 17.4 +26 19 51 23 54 17.7 +26 19 52 7485 289 3 1.99 0.08 13.5 1.94 102.0 9.69 1 2-477 333219 23 55 16.6 +27 27 29 23 55 16.0 +27 27 36 9229 264 9 1.27 0.09 8.2 2.13 127.0 9.68 1 2-478 333220 23 55 27.8 +27 59 23 23 55 29.3 +27 59 01 9015 116 11 0.91 0.06 10.0 1.88 123.9 9.52 1 2-479 331021 23 56 34.4 +27 11 41 23 56 34.4 +27 12 03 7905 333 4 2.54 0.10 14.3 2.17 108.1 9.85 1 2-480 12855 23 56 39.5 +27 06 28 23 56 37.3 +27 06 15 7875 420 1 2.00 0.11 10.0 2.12 107.6 9.74 1 2-481 331392 23 57 26.6 +26 49 58 23 57 25.8 +26 50 18 7679 282 5 2.74 0.09 16.7 2.18 104.8 9.85 1 2-482 333221 23 58 20.5 +27 16 45 23 58 21.5 +27 16 59 2900 96 6 0.94 0.06 9.6 2.21 41.0 8.57 1 2-483 12873 23 58 31.9 +26 12 50 23 58 32.1 +26 12 50 3250 131 1 4.11 0.06 38.2 2.10 46.0 9.31 1 2-484 333222 23 58 37.0 +27 30 59 23 58 36.9 +27 31 21 7295 118 7 1.33 0.05 14.2 1.92 99.4 9.49 1 2-485 333223 23 58 38.7 +26 49 50 23 58 40.3 +26 49 51 16860 83 3 0.74 0.06 8.2 2.21 236.0 9.99 1 2-486 12874 23 58 41.3 +27 08 15 23 58 41.9 +27 07 56 11616 236 5 1.50 0.08 10.9 2.01 161.1 9.96 1 2-487 333224 23 59 23.8 +26 32 51 23 59 24.2 +26 32 53 7717 161 5 1.14 0.07 9.7 2.06 105.4 9.48 1 2-488 331052 23 59 44.4 +27 15 28 23 59 45.0 +27 15 14 4692 61 2 0.56 0.04 7.6 1.87 66.5 8.77 1