These objects or files are not included in the HST.4web *? are " we did not analyze it" is may not mentioned in the paper QSO zem Reasons ========== ======= ==================================================== q0002p0507 1.90 h190 and h270a are spectropolarimetry. h270 is good. q0059m2735 1.596 BAL q0113p3249 0.016 h270 SPECTROPOLARIMETRY & does not include Lya. Not analyzed. no use. q0117p2118 h190,h270a SPECTROPOLARIMETRY q0119m0437 1.925 h190 is low S/N not reduced. h270 is good. q0150m2015 2.139 h190 is low S/N. not reduced. q0226m1024 2.256 BAL q0254m3327C 1.863 BAL q0256p3637 0.012 h270 SPECTROPOLARIMETRY not analyzed. no use. q0453m4220 2.66 h190 noisy not processed. h270 is good. q0743m6719 1.511 h190 and h270a SPECTROPOLARIMETRY. h270 is good. q0851p2017 0.306 BL Lac h190b( no line?) and h270a(SPECTROPOLARIMETRY) are not reduced. h270 is good. q0903p1734 2.771 BAL q0932p5006 1.920 BAL q0946p3009 1.216 BAL q1101p3828 0.031 BL Lac no emission. not analyzed. no use. q1120p0154 1.465 BAL q1146p1111 0.863 BAL q1213m0017 2.69 BAL q1216p5032b 1.451 BAL q1222p2251 --h270 SPECTROPOLARIMETRY q1246m0542 2.236 BAL q1254p0443 1.024 BAL q1254p5708 0.042 BAL q1309m0536 2.188 maybe BAL? low S/N. no use. q1354p2552 2.032 BAL q1402p4341 h270 SPECTROPOLARIMETRY q1411p4414 0.089 BAL q1413p1143 2.551 h270 is Messy spectrum.no use. q1524p5147 2.860 BAL q1535p5443 0.039 h190,h270 are SPECTROPOLARIMETRY.no use. q1615p3229 1.681 radio source --taken out q1634p7037 1.337 h190,h270a are spectropolarimetry. h270 is good. q1652p3950 0.033 h190,h270 SPECTROPOLARIMETRY.Not analyzed. no use. q1700p5153 0.288 BAL q1700p6416 2.722 h130 noisy spectra. Not analyzed. h190,h190a.h270 are ok. q1717p4901 0.025 h130 is low S/N. and not processed.h190,h270 are ok. q2302p0255 1.052 BAL ============================================================================ Notes: q0115p0242 --h270 no significant line q1202p2810 --h190 " q1401p0952 --h190 " q1545p2101 --h190 " These objects are fixed q0405m1219 --h130 new offset = -0.2376 *g fixed q0454p0356 --h190, h270 no change in offset *g fixed too q0955p3238 --h130 fixed continuum q1001p2910 --h270 fixed continuum fixed *g fixed too q1104m1805a --h270 " q1122m1648 --h190 " q1124p2711 --h270 " offset = -1.6052 q1148p5454 --h130 fixed continuum q1219p0447 --h130 " offset = 0.1177 q1222p2251 --h270 fixed continuum q1253m0531 --h130 fixed continuum q1351p6400 --h130 fixed continuum q1444p4047 --h270 fixed continuum q1517p2356 --h270 " h190 add continuum. use all.ps.pro.old( .sls) q1545p2101 --h130 " q2135m1446 -- h130,h190 continuum fixed q2216p0350 --h190 add continuum. use all.ps.pro.old( .sls) q2251p1120 --h130 fixed continuum new offset = 0.6036 BALq2302p0255 -h190, h270 fixed. h270b renamed as h270. use all.ps.pro.old( .sls) 0703/01 Additional fix. q0003p0146 0.234 h190 reduced. no significant line. q0050p1225 0.061 h190a,b,h270a,b,c do not include Lya. reduced. rename h190b --- h190 h270b --- h270 h270c --- h270b h130 is good.x q0052p2509 0.155 h190 does not include Lya. reduced. q0125m0635 0.005 h190 does not include Lya. reduced. q0150m2015 2.139 h270 does not include Lya. reduced. q1156p6311 0.594 h270 does not include Lya. reduced. q1306p3021 0.806 h270 does not include Lya. reduced. q1307p0835 0.155 h190 does not include Lya. reduced. q1311p0217 0.306 h190 does not include Lya. reduced. q1317m0142 0.255 h190 does not include Lya. reduced. q1415p4343 0.002 h190 does not include Lya. reduced. q1425p2003 0.111 h190 does not include Lya. reduced. q1612p2611 0.131 h190 does not include Lya. reduced. q1700p6416 2.722 h190,h190a,h270 do not include Lya. reduced. q1717p4901 0.025 h190 and h270 do not include Lya. reduced. q1928p7351 0.302 h190,h270 do not include Lya.reduced. q2349m0125 0.174 h190 no Lya. reduced. 3c273 h190 the ones we had were spectropolarimetry. Row Mark Targname RA Dec Aper Dataset Name Generation Date Archive Date Filters/Gratings Row 1 PG1226+023 12 29 06.70 +02 03 08.00 4.3 Y0G40206T Jun 20 1994 3:35:38AM Jun 20 1994 6:02:40PM G190H 1 2 PG1226+023 12 29 06.70 +02 03 08.00 1.0 Y0G40207T Jun 20 1994 1:58:57AM Jun 20 1994 2:00:44PM G190H 2 3 PG1226+023 12 29 06.70 +02 03 08.00 0.5 Y0G40209T Jun 20 1994 3:56:01AM Jun 20 1994 7:21:25PM G190H 3 4 PG1226+023 12 29 06.70 +02 03 08.00 0.3 Y0G4020BT Jun 20 1994 3:35:38AM Jun 20 1994 6:07:41PM G190H 4 5 PG1226+023 12 29 06.70 +02 03 08.00 0.3 Y0G4020CT Jun 20 1994 1:58:57AM Jun 20 1994 2:01:59PM G190H 5 6 PG1226+023 12 29 06.70 +02 03 08.00 0.25X2.0 Y0G4020PT Jun 20 1994 3:56:01AM Jun 20 1994 7:29:21PM G190H 6 7 3C273 12 29 06.71 +02 03 07.90 4.3 Y0NB0103T May 15 1998 5:00:59PM May 15 1998 5:54:01PM G190H 7 8 3C273 12 29 06.71 +02 03 07.90 4.3 Y0NB0105T May 15 1998 7:21:09PM May 15 1998 7:38:25PM G190H 8 1,4,6---Exp.flag INCOMPLETE 2,3,5--- only [1856 pix] instead of [2064] 7,8 --- spectropolarimetry 07/10/01 a,b,c files q0026p1259 -- h130a reduced Xq0405m1219 -- h130a spectropolarimetry q0414m0601 -- h190a,h270a reduced Xq0454m2203 -- h190a,h270a A-1 q0454p0356 -- h270a reduced Xq0624p6907 -- h190a,h270a Both noisy spectra Xq0907m0920 -- h270a noise Xq0923p3915 -- h190a,h270a,A-1 Xq1028p3118 -- h190a noise Xq1137p6604 -- h190a,h270a,A-1 Xq1146p1111 -- h190a BAL q1202p2810 -- h190a,h270a reduced Xq1211p1419 -- h190a,h270a both A-1 Xq1222p2251 -- h190a spectropolarimetry Xq1253m0531 -- h190a low S/N Xq1338p4138 -- h190a spectropolarimetry q1354p1933 -- h190a,h270a reduced q1402p2609 -- h190a,b reduced Xq1517p2357 -- h190a, noise Xq1521p1009 -- h270a A-1 h190a,h270b,spectropolarimetry Xq1544p4855 -- h130a noise Xq1618p1743 -- h190a,h270a both are A-1 Xq1641p3954 -- h190a,h270a,spectropolarimetry q1718p4807 -- h190a,h270b,spectropolarimetry, h270a reduced Xq2141p1730 -- h130a,h190a, both are A-1 Xq2155m3027 -- h130a spectropolarimetry Xq2216m0350 -- h190a,b,c,h270b,c all A-1 Xq2251p1120 -- h130a, A-1 q2251p1552 -- h190a,h270a reduced--h190b,h270b spectropolarimetry Xq2302p0255 -- h270a BAL q2340m0339 -- h270a reduced-h270b noise *run hst_ps.pro for the reduced spectra *ftp to tenmon HStfinal3.5, pclist.all *redo HST.4web *redo figure1