#Table: J/ApJS/97/1/./notes.dat (cdsarc.u-strasbg.fr) -------------------------------------------------------------------------------- No| te| No|Text --|----------------------------------------------------------------------------- 1|Quasar lies on or near an HVC listed in Table 3. 2|Wide-band or narrow-band HI measurements detect gas with |V_LSR_|>100km/s 2|(see V- and V+ above and Table 2). 3|V-emission may extend to -85km/s (UM 341). 4|V+ includes HVC at 111.5km/s (PKS 1101-32). 5|Apparent emission extending to +80km/s probably not real (PKS 1103-00, MC 5|1104+167, and PKS 1424-11). 6|Apparent emission extending to 90km/s probably not real (B2 1208+32A). 7|Also has HVC at -207 and -198km/s (Mrk 205). 8|Emission wing extending to 50km/s probably not real (T 1542). 9|Emission may extend to 80km/s (PKS1252+11). 10|V- and V+ are averages of two observing sessions (NGC1275). 11|Possible emission to -120km/s (KAZ 102). 12|Because of the large value of T_b_(max), the line core can not be properly 12|corrected for the effects of stray radiation. In Fig.1 we display the 12|uncorrected data in the upper panel and the corrected data in the lower panel 12|(PG 2112+059). 13|Emission may extend to -185km/s (3C 263.0). 14|Stray radiation removal process introduces emission near -90km/s (OJ 287). 15|Stray radiation removal process introduces emission near 60km/s (PG 15|1402+261). 16|Because of the large value of T_b_(max), the line core can not be properly 16|corrected for the effects of stray radiation. The uncorrected data which are 16|displayed in Fig.1 are reliable in the core but unreliable in the faint 16|wings. The corrected data were used to derive V- and V+ (3C 120). 17|Site line intersects a molecular cloud. E(B-V) from H I is therefore a lower 17|limit (3C 454.3). 18|Because of a telescope pointing error, the position actually observed 18|(RA=11h19m10s9 and DE=12deg10'42") differs by approximately 10' from the 18|correct position. --------------------------------------------------------------------------------