4-  1 HVC: small cloud.
4-  2 HVC: small cloud.
4- 10 HVC: small, isolated cloud.
4- 14 HVC: smaller, relatively isolated cloud in a densely populated region.
4- 18 HVC: bright knot of a larger cloud in a densely populated region.
4- 20 HVC: bright knot in an elongated filament in a densely populated region.
4- 23 HVC: bright knot in filament in densely populated region.
4- 28 HVC: more isolated cloud in velocity, but near a densely populated region.
4- 29 HVC: bright peak in a large cloud in a densely populated region.
4- 30 HVC: bright knot in HVC field/filament.
4- 32 HVC: small knot in relatively dense field.
4- 34 HVC: elongated cloud in somewhat dense field.
4- 39 HVC: small, isolated cloud.
4- 42 HVC: large, elongated cloud.
4- 44 HVC: cloud in dense region.
4- 45 cz mismatch with previous detection (Lawrence et al. 1999), but within 
4- 45  quoted measurement error.
4- 47 HVC: small, more isolated cloud near somewhat dense region.
4- 52 poor width precision due to shape of H i profile and poor spectral 
4- 52  definition.
4- 53 signal merges into strong RFI, severely affecting parameters.
4- 55 blend of emission from AGC320702 (224005.8+244156) and 
4- 55  AGC320701 (223957.0+244139); not separable spatially or kinematically. 
4- 55   Parameters uncertain.
4- 58 HVC: small cloud.
4- 59 HVC: small, relatively isolated cloud not far from some others.
4- 60 HVC: small, relatively isolated cloud in a field with several others.
4- 62 HVC: clumpy/patchy cloud in a region near others.
4- 70 HVC: bright knot in elongated filament in densely populated region.
4- 71 HVC: bright knot in elongated filament in densely populated region.
4- 73 HVC: bright peak in elongated cloud, in densely populated region.
4- 75 HVC: bright peak in cloud complex.
4- 76 HVC: bright peak in cloud complex.
4- 77 HVC: bright knot in cloud complex.
4- 78 HVC: bright knot in cloud complex.
4- 80 HVC: bright knot in elongated filament, part of a larger cloud complex.
4- 86 blend with emission from UGC12290; deblending good, but centroiding and 
4- 86  parameters for AGC320603 moderately uncertain.
4- 91 alternative opt.id with 230003.9+253359 (extremely LSB); position poorly 
4- 91  determined. Associated with group SRGb016 (Mahdavi et al. 1999).
4- 93 alternative opt.id with 230038.4+244704.
4- 99 blend of emission from two nearby galaxies; deblending not possible. 
4- 99  Lower-velocity emission is likely from the small nearby galaxy at 
4- 99   230212.7+244549; most of the emission is from the larger source.
4-101 HVC: small cloud.
4-103 HVC: small cloud.
4-106 double system with partial deblending: detection includes some flux from 
4-106  neighbor, UGC12386. Parameters and centroiding affected.
4-107 double system with partial deblending: detection includes some flux from 
4-107  neighbor, UGC12384. Parameters and centroiding affected.
4-111 HVC: large cloud.
4-118 blend with emission from nearby AGC330159 (231529.1+250714); not separable
4-118  spatially or kinematically. Parameters uncertain.
4-123 blend with emission from AGC330217 (231840.2+251601) to the north and 
4-123  signs of interaction. Parameters and centroiding affected.
4-125 HVC: elongated cloud.
4-128 HVC: small clump; somewhat difficult to distinguish from bulk of Galactic
4-128 HI emission.
4-136 note narrow profile width for object at cz=9700km/s.
4-141 HVC: small isolated cloud.
4-148 blend with emission from AGC331873 (232601.0+254137); signal merges into 
4-148  strong RFI, affecting parameters on high cz end of profile; deblending 
4-148   poor due to spatial and kinematic overlap.
4-150 HVC: small clump; somewhat difficult to distinguish from bulk of Galactic
4-150  HI emission.
4-179 near region of poor spatial and spectral coverage; affects centroiding and
4-179  distance between H i center and opt.id.
4-183 poor spectral definition on low-cz end of profile.
4-188 opt.id's appear to be an interacting system.
4-193 poor spectral definition, with ambiguous opt.id: possible alternative id 
4-193  with 234528.5+241303 and 234526.8+241307; emission may be a blend from 
4-193   all three.
4-195 HVC: large cloud; somewhat difficult to distinguish from bulk of Galactic
4-195  HI emission.
4-204 HVC: small cloud.
4-207 possible alternative opt.id with 235449.2+245058, but less likely.
4-208 blend of AGC331012 with AGC331014 (235548.1+253031) and 
4-208  331015 (235551.8+252933); no deblending. Parameters uncertain: signal is
4-208   intrinsically broad, but also merges into RFI and approaches end of 
4-208    ALFALFA bandwidth.
4-209 HVC: isolated large cloud.
4-216 HVC: small, isolated knot.
4-220 UGC94 nearby at same cz; deblending good, parameters mostly unaffected.
4-221 UGC89 nearby at same cz; deblending good, parameters mostly unaffected.
4-222 HVC: small, isolated cloud.
4-225 possible alternative opt.id with 001034.8+243005, farther from H i center.
4-227 poor spectral definition (high noise).
4-228 significant polarization mismatch.
4-234 possible alternative opt.id with 001611.8+245211.
4-237 parameters affected by proximity to AGC100146 (001759.7+243345).
4-238 parameters affected by proximity to UGC165.
4-241 HVC: bright knot of a larger cloud.
4-248 opt.id ambiguous; other possible counterpart at 002258.5+254723 but 
4-248  farther from HI center.
4-249 near border of region; detection and parameters will be improved once data
4-249  are available for +23 degree strip to the south.
4-255 HVC: bright knot of a larger cloud extending to the east.
4-257 HVC: bright knot.
4-260 HVC: bright knot of a much larger complex of clouds.
4-261 unresolved broad blend of emission from HCG 001. Centered on UGC248 pair 
4-261  (disturbed optical morphology); blend of flux from group, with uncertain
4-261   parameters. Not separable spatially or kinematically.
4-268 HVC: bright knot in an extended filament/cloud structure.
4-269 HVC: bright knot in a much larger complex of clouds.
4-272 HVC: bright knot in a much larger complex of clouds.
4-277 HVC: bright knot in a much larger complex of clouds.
4-280 possible alternative opt.id with 003237.2+244854, but much less likely.
4-281 HVC: one of the many knots in this densely populated region.
4-285 HVC: one of the many knots in this densely populated region.
4-286 HVC: one of the many knots in this densely populated region.
4-287 opt.id is distant (1.6arcmin), but has previous optical redshift 
4-287  measurement of cz=9838km/s.
4-290 HVC: one of the many knots in this densely populated region.
4-292 signal merges with strong RFI; parameters uncertain.
4-294 HVC: one of the many knots in this densely populated region.
4-298 opt.id ambiguous; other possible counterpart at 003828.2+253616.
4-308 parameters affected by poor coverage in this region.
4-313 possible alternative opt.id with 004433.2+254143.
4-317 blend with AGC100511 (004557.3+251308); significantly broadens the profile
4-322 alternative opt.id with 004842.0+243554; flux may be a blend.
4-324 HVC: one of two measured peaks in a large cloud in this densely populated
4-234  region.
4-327 blend of emission from AGC100594 and AGC100596 (005025.6+243114); not 
4-327  separable spatially or kinematically.
4-330 HVC: bright peak near a filament that blends into Galactic emission.
4-336 blend of emission from AGC101857 and AGC101858 (005456.4+255308); not 
4-336  separable spatially or kinematically.
4-337 HVC: bright peak in a densely populated region.
4-339 HVC: isolated, small cloud in a densely populated region.
4-342 alternative opt.id with 005629.1+241911.
4-343 HVC: larger cloud in a densely populated region.
4-344 HVC: compact cloud in a densely populated region.
4-346 HVC: bright peak in a large cloud, distinct from Galactic emission.
4-352 HVC: large cloud of emission, not entirely spectrally distinct from bulk 
4-352  of Galactic HI emission.
4-354 alternative opt.id with 010555.1+243435; emission may be a blend of both.
4-355 poor centroiding; galaxy emission plus a low-level emission extended in 
4-355  redshift space. Identified as AGC110025, but some emission is likely to
4-355   be associated with nearby galaxies at 010619.0+253212.3 and 
4-355    010617.4+253342.9. Unmeasured broader emission covers 6330-6600km/s, 
4-355     and the measurement of AGC110025 likely contains some contamination 
4-355      from this additional gas.
4-358 HVC: subclump of Wright's Cloud complex.
4-359 HVC: subclump of Wright's Cloud complex.
4-360 HVC: entirety of the Wright's Cloud clump in +25deg region. Contains many
4-360  subclumps which were measured separately; bulk of the cloud extends into
4-360   +27deg region (see Saintonge et al., 2008, Cat. J/AJ/135/588).
4-361 HVC: small clump, part of Wright's Cloud complex.
4-362 HVC: possibly an unusual positive velocity cloud. Significant polarization
4-362  squint; caution as signal may be spurious.
4-364 signal merges with strong RFI; parameters affected and some flux lost.
4-365 HVC: clump in an area with several more clouds.
4-368 HVC: clump in an area with several more clouds.
4-372 interacting triplet: UGC884, AGC113819 (012059.7+253207), and AGC110845 
4-372  (012052.9+253247). Likely to be at a lower velocity; RFI strongly affects
4-372   profile and parameters. Actual velocity width of emission closer to 
4-372    400km/s.
4-377 HVC: large isolated cloud.
4-378 HVC: one of two clumps in a small faint cloud.
4-379 HVC: one of two clumps in a small faint cloud.
4-380 signal merges with strong RFI; parameters uncertain.
4-381 HVC: the brightest of several small distinct clouds in this region.
4-384 HVC: one of the small clouds in this region.
4-386 HVC: one of the small clouds in this region.
4-388 opt.id ambiguous: second possible counterpart at 013744.3+243153.
4-389 HVC: cloud not completely spectrally distinct from bulk of Galactic HI 
4-389  emission.
4-390 HVC: companion to cloud HI013806.2+245528, not completely spectrally 
4-390  distinct from bulk of Galactic HI emission.
4-395 possible alternative opt.id with AGC113308 (014429.3+255114, no previous 
4-395  cz), but associated with AGC113307 because of match with previous 
4-395   measurement.
4-397 opt.id ambiguous; other possible counterpart at 014509.6+245535.
4-401 opt.id ambiguous; other possible counterpart at 014619.6+252140.
4-412 HVC: cloud not completely spectrally distinct from bulk of Galactic HI 
4-412  emission.
4-417 flux much larger than previous measurements (available through our public
4-417  digital archive site).
4-432 HVC: clumpy, irregular shape, well separated spectrally from galactic HI.
4-432  Extends about half a degree; may extend into unavailable region to the
4-432   south at +23deg.
4-440 HVC: central and brightest region of a filament that extends for over 2deg
4-441 alternative opt.id with 021303.9+252126.
4-446 HVC: group of knots.
4-447 parameters uncertain; signal may be contaminated by AGC121503 
4-447  (021610.7+251413). Deviation from 2-horn profile shape and possible 
4-447   signs of interaction.
4-448 parameters uncertain; signal may be contaminated by UGC1739. Deviation 
4-448  from 2-horn profile shape and possible signs of interaction.
4-449 no discernible optical counterpart.
4-450 HVC: one of the many knots in this densely populated region.
4-451 HVC: patchy cloud that may extend farther south into unavailable region 
4-451  at +23deg.
4-452 galaxy shows clear signs of interaction: optical morphology very 
4-452  irregular, and presence of an extension of the HI, wider than the main 
4-452   emission from the galaxy.
4-453 HVC: one of the many knots in this densely populated region.
4-456 HVC: one of the many knots in this densely populated region.
4-458 HI disk seems elongated toward the NW, low surface brightness extension 
4-458  to one side of the galaxy.
4-460 asymmetric shape (both H i and optical image).
4-461 HVC: one knot in one of the filaments that extends to the east of 
4-461  HI022823.7+244309.
4-464 HVC: elongated filament.
4-473 parameters uncertain because of low S/N.
4-474 opt.id ambiguous; other possible counterpart AGC122812 (022606.5+255855).
4-476 possible alternative opt.id with AGC122133 (022646.8 +244236), but more 
4-476  than 2 arcmin from HI centroid.
4-483 HVC: bright central knot of system of filaments that extend throughout 
4-483  the grid.
4-486 opt.id ambiguous; other possible counterpart (or blend of emission) at 
4-486  022908.9+251808. Parameters uncertain.
4-487 HVC: one knot in one of the filaments that extends to the north of 
4-487  HI022823.7+244309.
4-491 parameters affected by high noise; width determination uncertain.
4-499 alternative opt.id twice the distance away at 023528.2+253343.
4-503 outer isophotes asymmetrical, distribution appears to stretch to the east.
4-504 possible alternative opt. id with 024124.5+241627, similar galaxy but more
4-504  than 1arcmin away.
4-506 possible alternative opt. id with 024154.6+245657, but about 1arcmin 
4-506  farther away from HI center.
4-523 HVC: small cloud.
4-528 parameters uncertain; signal partly blended with AGC120695 
4-528  (025804.1+252656). Width could be larger that what is measured here.
4-529 parameters uncertain; signal partly blended with AGC120678 
4-529  (025759.1+252526).
4-534 HI disk is elongated; appears affected by two nearby neighbors AGC120727 
4-534  (025818.1+252657) and UGC2442.
4-540 HI emission links this galaxy with UGC2457, 10 arcmin north.