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Sorted By :	Subject	Author	Quasars	Other Objects	All Abstracts

QUASAR CROSS REFERENCE

Observation Type:

ROSAT= X-Ray image from the Roengten Satelit

VLBA = Very high resolution radio image from the Very Long Baseline Array

VLA = Very Large Array images

NRAO = Radio image on CDROM from the National Radio Astronomy Observatory

LBQS = Optical data from the Large Bright Quasar Survey (spectra)

0002-422
- Contains more than 10 absorption lines and 3934 Ca II and 3934 Ca II
0003-003 (3CR 2)
- z=1.037, group 17
0017+154 (3CR 9)
- z=2.012, group 28
- 3663 Å (no Lyman continuum absorption shortwards)
- Contains more than 10 absorption lines
0024+224
- z=1.118, group 18
- group 18
0029+002 (UM 253)
- 0237-233 family. Close member with 0028+002 (62 arcsec). Missing Lyman alpha paradox !
- 0237-233 family. Emission lines X,2,3,4,X,6 at 3994, 4507, 4991 and 6160 Å
- 0237-233 family. Line 1 absent and line 2 present the opposite of 0237-233
- LBQS spectra (0029+0017) page 1977 from Foltz et al. (1989)
0038-019
- z=1.690, group 52
0045-036 (UM 667)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0046+154 (PHL 847)
- z=1.243, group 47
0047-832
- group 18
0050+106 (PHL 881)
- z=0.321, group 33
0051-279 (S93)
- C III 6730, 6744 Å and C II 8413 Å emission. Ly-alpha absent ! Predict C III 4650 Å.
0052+145 (PHL 892)
- z=0.911, group 14
0056-001 (PHL 923)
- z=0.717, group 11
- LBQS spectra (0056-0009)
0056+126 (PHL 921)
- z=1.088, group 46
0058+019 (PHL 938)
- 3C 191, PHL 938, PKS 0119-04, BO 6 group
- z=1.9552, group 27
- Contains more than 10 absorption lines and 3934 Ca II
- LBQS spectra (0058+0155)
0100+130 (PHL 957)
- Identification of 3889 Å He II shell star absorption line and WU level absorption hole at 4020 Å
- 3389 (He I, Shell)
- Contains more than 10 absorption lines and 3934 Ca II
0107-156
- z=0.861, group 12
0114-089 (UM 670)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0116-288
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0119-046
- 3C 191, PHL 938, PKS 0119-04, BO 6 group
- z=1.955, group 27
- Contains more than 10 absorption lines
0122-003
- z=1.070, group 45
0123+257 (4C 25.05)
- Identification of 3889 Å He II shell star absorption line
- 3389 Å (He I, Shell)
- Contains more than 10 absorption lines
0128+074 (PHL 3375)
- Proper motion of 5.8±18 milliarcsec/yr
0130+033 (PHL 1027)
- z=0.363, group 35
- Proper motion of 16.6±13 milliarcsec/yr
0131+037 (PHL 1033)
- Significant proper motion, 0.05 arcsec/yr
- Significant proper motion, 0.05 arcsec/yr
- Proper motion of 48.8±13 milliarcsec/yr
- z=0.255, group 32
0131+055 (PHL 3424)
- Proper motion of 12.0±18 milliarcsec/yr
0132-197 (UM 672)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0132+077 (PHL 1049)
- Proper motion of 21.8±13 milliarcsec/yr
0133+207 (3CR 47)
- z=0.425, group 7
- Double-lobes
- ROSAT (Feb 1 1992, 5105 sec., p700069) 01 36 24.00 20 57 36.00
0134+329 (3CR 48)
- Population inversion in 4686 Å He II
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
- ROSAT (Jan 26 1992, 5692 sec., rp700328) 1 37 40.80 33 9 36.00
- VLBA Conway, Pearson, Ojha
0135-002 (UM 349)
- 0237-233 family. Emission lines 1,X,X,4,X,X at 3900 and 500 Å
0135+056 (PHL 1072)
- z=0.615, group 36
- Proper motion of 28.6±13 milliarcsec/yr1
0137+012 (PHL 1093)
- z=0.262, group 1
- ROSAT (Jul 14 1993, 15584 sec., rp701407n00) 01 39 57.00 +01 31 48.0
0137+060 (PHL 1092)
- Proper motion of 17.5±13 milliarcsec/yr
- ROSAT (Jan 19 1992, 8068 sec.?, p700259 ?) 01 39 55.20 06 19 12.00
0138-381 (MD2:62)
- 0805+046 family. Helium-rich shell star, 4713.14 He I emission, evidence of abs. lines
- 0805+046 family. Emission lines 1,2,3 at 4703, 5428 and 5996 Å
0139+059 (PHL 1106)
- Proper motion of 32.3±13 milliarcsec/yr
0139+061 (PHL 3632)
- Proper motion of 25.1±18 milliarcsec/yr
0140-306
- 0420-388 family.
- 0420-388 family. Emission lines at X,2,X,X,5 at 5020 and 6370 Å
- 0420-388 family. Helium discontinuity at 3665 Å
0140+081 (PHL 1119)
- Proper motion of 23.3±13 milliarcsec/yr
0141+052 (PHL 1127)
- Proper motion of 21.2±13 milliarcsec/yr
- z=1.985, group 56
0141+339 (4C 33.03)
- O VI sequence quasar
- 3811+3834 (O VI), 4658 (C IV), 4686 (He II)
0143-015 (UM 366)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0143-010 (UM 368)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0147+089 (PHL 1186)
- Proper motion of 18.4±13 milliarcsec/yr
0148+090 (PHL 1194)
- z=0.299, group 2
- Proper motion of 26.2±13 milliarcsec/yr
0151+045 (PHL 1226)
- z=0.404, group 5
- Proper motion of 1.0±13 milliarcsec/yr
0151+048 (PHL 1222)
- RS 23, PHL 1222, 1548+115b group
- z=1.910, group 26
- Proper motion of 4.2±13 milliarcsec/yr
- Contains more than 10 absorption lines
0202+319
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
0205+024
- Similar to spectra of 3C 273
- ROSAT (Jan 23 1992, 7835 sec., f700432) 02 07 50.40 02 43 12.00
- ROSAT (Jan 18 1992, 14070 sec., p700432)
0226-038 (PHL 1305)
- z=2.064, group 29
0229+131
- z=2.065, group 29
- VLBA Beasley, Clark
0232-042 (PHL 1377)
- 4652 Å C III Wolf-Rayet laser line
- ROSAT (Feb 5 1992, 10039 sec., rp700350) 2 35 7.20 - 4 1 48.00
0235+164
- (BL Lac object) no need of assuming redshift in spectra
- ROSAT (Aug 15 1993, 1708 sec., rp701388n00) 02 38 38.00 +16 37 12.0
- ROSAT (Jul 26 1993, 1508 sec., rp701381n00)
- ROSAT (Jul 21 1993, 2083 sec., rp701379n00)
- ROSAT (Jul 24 1993, 1903 sec., rp701380n00)
- ROSAT (Jul 29 1993, 1192 sec., rp701382n00)
- ROSAT (Aug 6 1993, 4099 sec., rp701385n00)
- ROSAT (Aug 4 1993, 2023 sec., rp701384n00)
- ROSAT (Aug 12 1993, 1664 sec., rp701387n00)
- ROSAT (Aug 1 1993, 1783 sec., rp701383n00)
- VLBA Beasley, Gwinn, Marscher
0237-233
- Identification of 14 He I absorption lines
- Hydrogen deficient shell star with He I, He II and O II lines
- Identification of 3889 Å He II shell star absorption line
- Chance coincidences
- 3389 (He I, Shell)
- Chance coincidences in C IV doublets absorption redshifts
- (or PHL 8462) proper motion of 23.6±13 milliarcsec/yr
- Contains more than 10 absorption lines and 3934 Ca II
- Chance coincidences in CO absorption redshifts
- 0237-233 family. Five emission lines found
- 0237-233 family. Emission lines 1,X,3,4,5,6 at 3930, 4537, 4993, 5285 and 6141 Å
- 0237-233 family. Identification of absorption lines
- 0237-233 family. Helium discontinuity at 2600 Å
- 0237-233 family. Similarity with Upsilon Sagittarii
0242-410
- 0237-233 family. Emission lines 1,2,X,4,5,6 at 3905, 3984, 4986, 5267 and 6155 Å
0242-301 (NGC 1097)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
- ROSAT (Dec 27 1992, 9638 sec., wp600449n00) 02 46 19.20 -30 13 12.0
0244-128
- 0237-233 family. Emission lines 1,2,3,4,5,6 at 3869, 3989, 4480, 4952, 5253 and 6120 Å
0316-203
- 0805+046 family. Helium-rich shell star, 4713.14 He I emission, evidence of abs. lines
- 0805+046 family. Emission lines 1,2,3 at 4750, 5411 and 5957 Å
0317-023 (4C 02.15)
- z=2.092, group 31
0334-204 (UM 683)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0348+061
- z=2.058, group 29
0349-146 (MSH 03-19)
- z=0.614, group 36
0350-073 (3C 94)
- z=0.962, group 15
0403-132
- z=0.571, group 10
- VLBA Wardle 01/06/96
0414-060
- z=0.781, group 39
0420-388
- 0420-388 family. Equivalent width of line 2 and 3 is 132 Å
- 0420-388 family. 1,2,3,4,X at 4250, 5013, 5100 and 5800 Å
- 0420-388 family. Identification of 186 absorption lines
- 0420-388 family. Helium discontinuity at 3760 Å
- ROSAT (Feb 20 1991, 15611 sec., p700026) 04 22 14.40 -38 45 00.00
0420+003
- 0805+046 family. Helium-rich shell star, 4713.14 He I emission
0424-131
- z=2.165, group 57
- Contains more than 10 absorption lines and 3934 Ca II
0453-423
- Contains more than 10 absorption lines
- ROSAT (Jan 15 1992, 3161 sec. ?, p400163) 04 53 00.00 -42 13 48.00 (RX J0453-4214)
0457+024 (OF 097)
- Contains more than 10 absorption lines and 3934 Ca II
0528-250
- Contains more than 10 absorption lines
0537-286
- Contains more than 10 absorption lines
- 0420-388 family. 22 absorption lines
- 0420-388 family. 1,2,3,4,5 at 4238, 5000, 5090, 5760 and 6302 Å
- 0420-388 family. Helium discontinuity at 3650 or 3633 Å
- ROSAT (Sep 28 1992, 9487 sec., wp701094n00) 05 39 55.20 -28 40 12.0
0642+449 (OH 471)
- Contains more than 10 absorption lines
0736-063
- Contains more than 10 absorption lines
0738+313 (OI 363)
- z=0.630, group 37
0740+380 (3CR 186)
- z=1.063, group 44
0751+298 (4C 29.27)
- z=0.363, group 35
0801+303 (4C 30.13)
- z=1.446, group 50
0802+103 (3CR 191)
- 3C 191, PHL 938, PKS 0119-04, BO 6 group
- z=1.956, group 27
- Contains more than 10 absorption lines and 3934 Ca II
0805+046 (4C 05.34)
- Hydrogen deficient shell star with He I, He II and O II lines.
- Absorption-line red-shifts are meaningless
- Absorption-line red-shifts are meaningless
- Absorption-line red-shifts are meaningless
- Contains more than 10 absorption lines
- He I 4713 Å emission line, helium discontinuity at 3422 Å, He II and Fe II absorption lines.
- 0805+046 family. Helium-rich shell star, 4713.14 He I emission (nova line) and 3422 He discontinuity
- 0805+046 family. Emission lines 1,2,3 at 4714, 5424 and 6004 Å
- 0805+046 family. Identification of absorption lines
- Data quality problems in spectra are similar to 0237-233
- Chance coincidences
0812+020
- z=0.402, group 5
0824+110
- Contains more than 10 absorption lines and 3934 Ca II
0830+115
- Contains more than 10 absorption lines and 3934 Ca II
0833+654 (3CR 204)
- z=1.112, group 18
- group 18
- 4030, 3275 Å
0834+250 (OJ 259)
- group 18
0835+580 (3CR 205)
- z=1.534, group 51
- VLBA Lonsdale
0836+195 (4C 19.31)
- z=1.689, group 52
0843+136 (4C 13.39)
- z=1.875, group 25
0844+319 (4C 31.32)
- z=1.834, group 54
0846+100 (4C 09.31)
- Population inversion in 4686 Å He II
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
0847+190 (LB 8741)
- Proper motion of 17.9±18 milliarcsec/yr
0848+155 (LB 8755)
- z=2.010, group 28
0848+163 (LB 8775)
- Proper motion of 5.1±18 milliarcsec/yr
- ROSAT (Apr 23 1993, 3925 sec., rp700818n00) 08 51 40.00 +16 12 35.0
0850+140 (3CR 208)
- z=1.112, group 18
- 4030, 3275 Å
- group 18
- ROSAT (Nov 13 1992, 18552 sec., rp700887n00) 08 53 9.60 +13 52 48.0
- VLBA Hough 09/02/95
0851+197 (LB 8863)
- Proper motion of 15.3±18 milliarcsec/yr
- 0237-233 family. Emission lines 1,X,3,4,X,X at 3912, 4494 and 4972 Å
0852+181 (LB 8891)
- Proper motion of 15.8±18 milliarcsec/yr
0854+191 (LB 8948)
- z=0.331, group 34
- Proper motion of 17.9±18 milliarcsec/yr
- ROSAT (May 13 1992, 5150 sec., rp800134) 8 57 26.40 18 55 12.00
0854+191 (LB 8956)
- Significant proper motion, 0.06 arcsec/yr
- Significant proper motion, 0.06 arcsec/yr
- Proper motion of 60.8±18 milliarcsec/yr
0855+188 (LB 8991)
- z=1.013, group 43
- Significant proper motion, 0.05 arcsec/yr
- Significant proper motion, 0.05 arcsec/yr
- Proper motion of 50.5±18 milliarcsec/yr
0856+170 (4C 17.46)
- (LB 9013) Proper motion of 29.1±18 milliarcsec/yr
- z=1.444, group 50
0856+186 (LB 9010)
- Proper motion of 13.0±18 milliarcsec/yr
0856+189 (LB 9029)
- Proper motion of 36.1±18 milliarcsec/yr
0903+169 (3CR 215)
- (LB 9308) Proper motion of 20.1±18 milliarcsec/yr
- z=0.411, group 6
- ROSAT (Nov 18 1991, 6300 sec., p700385) 09 06 31.20 16 46 12.00
0906+015
- z=1.018, group 16
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
- VLBA Fomalont
0906+167 (LB 9388)
- Proper motion of 30.9±18 milliarcsec/yr
- z=1.070, group 45
0922+005
- z=1.720, group 53
0922+149
- z=0.896, group 13
0923+392 (4C 39.25)
- Similar to spectra of 3C 273
- ROSAT (May 1 1992, 1329 sec., f700505) 09 27 02.40 39 02 24.00
- ROSAT (May 1 1992, 6190 sec. ?, p700505)
- ROSAT (Apr 22 1993, 3585 sec., rp700848n00) 09 27 2.00 +39 02 24.0
- ROSAT (Apr 24 1993, 4174 sec., rp700849n00)
- ROSAT (Apr 26 1993, 4568 sec., rp700850n00)
- ROSAT (Apr 28 1993, 5136 sec., rp700851n00)
- ROSAT (Apr 30 1993, 5423 sec., rp700852n00)
- VLBA Alberdi, Beasley, Briggs, Clark, Flatters, Langevel, Marscher, Marcaide, Marvel, Moran, Romney
0926+117 (4C 11.32)
- z=1.754, group 23
0937+118
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0938+450 (US 844)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
0952+097 (4C 09.35)
- z=0.299, group 2
0952+357 (4C 35.21)
- z=1.241, group 47
0957+003
- z=0.907, group 14
- 3640, 5337 Å
0957+561
- Quasar association at 300 pc, group 20 (Varshni, 1976)
- ROSAT (Oct 22 1992, 18677 sec., rh700889n00 10 01 21.60 +55 54 0.0
- STScI grav.lens page
- Kundié,T., Colley,W.N., Gott,J.R., Malhotra,S., Pen,U-L, Rhoads,E., Stanek,K.Z., Turner,E.L., Wambsganss,J.: 1995, ApJ., 455, L5. Dec 1994-May 1995 photometry in quasar A predicts time delayed event in quasar B (microlensing is ruled out for this event)
0958+551 (MKN 132)
- Contains more than 10 absorption lines
- z=1.758, group 23
1001+226 (4C 22.26)
- z=0.974, group 42
1022+194 (4C 19.34)
- z=0.828, group 40
1023+067 (4C 06.40)
- z=1.69, group 22
1040+123 (3CR 245)
- Superluminal expansion
- ROSAT (Nov 19 1991, 10209 sec., p700384) 10 42 45.60 12 03 36.00
1045+604 (4C 60.15)
- z=1.722, group 53
1046+053 (4C 05.46)
- z=1.115, group 18
- group 18
1047+096 (4C 09.37)
- z=0.786, group 39
1049+616 (4C 61.20)
- z=0.422, group 7
1055+201
- z=1.110, group 18
- group 18
1058+110 (4C 10.30)
- z=0.423, group 7
1100+772 (3CR 249.1)
- z=0.31, group 3
- NRAO Images from the radio universe cd2:qsos/1100p772.
- VLBA Hough 09/02/95
1104+167 (4C 16.30)
- z=0.634, group 37
1111+408 (3CR 254)
- z=0.734, group 38
- ROSAT (May 18 1993, 16159 sec., rp700855n00) 11 14 38.00 +40 37 12.0
1124+571 (OM 540/4)
- 0805+046 family. Helium-rich shell star, 4713.14 He I emission
- 0805+046 family. Emission lines 1,2,3 at 4731, 5364 and 6023 Å
- VLBA Lonsdale
1126+101
- z=1.515, group 21
1132+303 (3C 261)
- 4515 Å N III Wolf-Rayet laser line
1136-135
- PKS 1136-12; 4349 Å O II Wolf-Rayet laser line.
1148-001
- z=1.982, group 56
- LBQS spectra (1148-0007)
- VLBA Claussen
1150+497 (LB 2136)
- z=0.334, group 34
- ROSAT (Dec 1 1992, 6610 sec., wp701073n00) 11 53 24.00 +49 31 12.0
- VLBA Bloom
1156+295 (4C 29.45)
- z=0.728, group 38
- VLBA Moellenb
1158+122
- Contains more than 10 absorption lines
- Identification of 3889 Å He II shell star absorption line
- 3389 Å (He I, Shell)
1203+109 (4C 10.34)
- z=1.088, group 46
1206+119 (H 51.2)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1206+439 (3CR 268.4)
- z=1.400, group 20
- VLBA Zensus
1218+339 (3CR 270.1)
- z=1.519, group 21
- ROSAT (May 23 1993, 19290 sec., rp700864a01) 12 20 33.00 +33 43 12.0
- ROSAT (Jun 20 1992, 3010 sec., rp700864)
1221+113
- 1221+11; z=1.755, group 23
1221+186 (4C 18.34)
- z=1.401, group 20
1222+216 (4C 21.35)
- z=0.433, group 8
1222+228 (TON 1530)
- Contains more than 10 absorption lines
- NRAO Images from the radio universe cd2:qsos/1222p228.
1225+317
- Contains more than 10 absorption lines and 3934 Ca II
- 0237-233 family. Emission lines 1,X,X,4,X,X at 3930 and 4950 Å
- ROSAT (Jun 5 1992, 1462 sec., wf700506) 12 28 24.00 31 28 48.00
- ROSAT (May 31 1992, 8820 sec., wp700506)
1226+023 (3C 273)
- Emission lines identified as 3229 Å O III and 7598 Å C III
- Superluminal expansion
- Radio/optical/uv spectrum resembles NGC 7027
- ROSAT (Dec 15 1991, 3293 sec., f700191) 12 29 04.80 02 03 00.00
- ROSAT (Dec 14 1991, 7249 sec.?, p700191)
- ROSAT (HRI 17174 sec., wh700234) 12 29 7.20 2 3 0.00
- ROSAT (Dec 22 1992, 1326 sec., wp701262n00)
- ROSAT (Jan 7 1993, 1973 sec., wp701255n00)
- ROSAT (Dec 20 1992, 1124 sec., wp701261n00)
- ROSAT (Dec 27 1992, 1705 sec., wp701264n00)
- ROSAT (Jan 9 1993, 2004 sec., wp701256n00)
- ROSAT (1473 sec., wh701257n00)
- ROSAT (Dec 18 1992, 1049 sec., wp701259n00)
- ROSAT (Dec 15 1992, 1042 sec., wp701258n00)
- ROSAT (Dec 18 1992, 1744 sec., wp701260n00)
- ROSAT (Dec 2 1993, 1874 sec., wp701267n00)
- ROSAT (Dec 31 1992, 1840 sec., wp701266n00)
- ROSAT (Dec 25 1992, 1503 sec., wp701263n00)
- ROSAT (Jan 5 1993, 1976 sec., wp701269n00)
- ROSAT (Dec 29 1992, 1786 sec., wp701265n00)
- ROSAT (Jan 3 1993, 1970 sec., wp701268n00)
- ROSAT (Jun 15 1993, 3332 sec., wp141509n00) 12 29 4.00 +02 03 0.0
- VLBA Baath, Beasley, Boboltz, Conway, Diamond, Junor, Leppanen, Lobanov, Marvel, Romney, Zensus,...
1226+105
- Contains more than 10 absorption lines
- LBQS spectra (1226+1035) page 1445 from Foltz et al. (1987)
1241+166 (3CR 275.1)
- z=0.557, group 9
1244+114
- (1244+1129) 0420-388 family. Visible absorption lines
- 0420-388 family. X,2,X,X,X at 5058 Å
- 0420-388 family. Helium discontinuity at 3720 Å
- LBQS spectra (1244+1129) page 1457 from Foltz et al. (1987)
- ROSAT (Dec 21 1991, 4177 sec., p700397) 12 46 40.80 11 13 12.00 (1244+1129)
1246-057
- 0237-233 family. Emission lines X,2,X,4,X,X at 3976 and 4983 Å
- Contains more than 10 absorption lines
- ROSAT (Dec 21 1991, 13405 sec., p700375) 12 49 14.40 -05 59 24.00 (Q1246-0542)
1246+377 (BSO 1)
- z=1.241, group 47
1248+305 (4C 30.25)
- z=1.061, group 44
1251+367
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1252+119
- z=0.871, group 41
1253-055 (3C 279)
- Superluminal expansion
- ROSAT (Jan 3 1992, 4230 sec., p700075) 12 56 12.00 -05 47 24.00
- ROSAT (Jan 2 1992, 4925 sec., p700305)
- ROSAT (Jan 2 1992, 8513 sec., rp700305)
- ROSAT (Jan 6 1993, 3925 sec., rp700989n00)
- ROSAT (Jan 12 1993, 4003 sec., rp700994n00)
- ROSAT (Jan 8 1993, 3860 sec., rp700990n00)
- ROSAT (Jan 2 1993, 3894 sec., wp701101n00)
- ROSAT (Jan 11 1993, 3384 sec., rp700993n00)
- ROSAT (Jan 5 1993, 2814 sec., rp700987n00)
- ROSAT (Dec 27 1992, 3228 sec., rp700978n00)
- ROSAT (Jan 6 1993, 2002 sec., rp700988n00)
- ROSAT (Jan 13 1993, 1969 sec., rp700995n00)
- ROSAT (Jan 3 1993, 3939 sec., wp701106n00)
- ROSAT (Jan 4 1993, 2006 sec., wp701111n00)
- ROSAT (Dec 28 1992, 3431 sec., rp700979n00)
- ROSAT (Jan 2 1993, 3489 sec., wp701105n00)
- ROSAT (Jan 5 1993, 3594 sec., wp701120n00)
- ROSAT (Dec31 1992, 1867 sec., rp700982n00)
- ROSAT (Dec 29 1992, 3688 sec., rp700980n00)
- ROSAT (Jan 3 1993, 3518 sec., wp701110n00)
- ROSAT (Jan 4 1993, 1973 sec., wp701113n00)
- ROSAT (Dec 30 1992, 3711 sec., rp700981n00)
- ROSAT (Jan 4 1993, 3800 sec., wp701116n00)
- ROSAT (Jan 9 1993, 3500 sec., rp700991n00)
- ROSAT (Jan 10 1993, 3897 sec., rp700992n00)
- ROSAT (Jan 5 1993, 3213 sec., wp701119n00)
- ROSAT (Jan 4 1993, 1752 sec., wp701115n00)
- ROSAT (Jan 2 1993, 3181 sec., wp701104n00)
- ROSAT (Jan 3 1993, 3213 sec., wp701109n00)
- ROSAT (Jan 2 1993, 1454 sec., wp701102n00)
- ROSAT (Jan 3 1993, 1835 sec., rp700985n00)
- ROSAT (Jan 4 1993, 3200 sec., wp701114n00)
- ROSAT (1393 sec., rp700984n00)
- VLBA Baath, Benson, Bloom, Claussen, Kellermann, Leppanen, Wehrle
1253+104
- z=0.824, group 40
1256+357 (B 194)
- z=1.876, group 25
- Contains more than 10 absorption lines and 3934 Ca II
1257+346 (B 201)
- z=1.375, group 49
1258+286 (5C4.127)
- z=1.373, group 49
1259+344 (BSO 6)
- z=1.956, group 27
- BO 6 ?; 3C 191, PHL 938, PKS 0119-04, BO 6 group
1306+294 (KKC 35)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1308+182 (4C 18.36)
- z=1.689, group 52
1311+362 (BSO 11)
- 3748 Å O II Wolf-Rayet laser line
- z=2.084, group 30
1317+520 (4C 52.27)
- z=1.060, group 44
1318+113 (4C 11.45)
- z=2.171, group 57
1318+290 (TON 155)
- z=1.703, group 22
1320-106 (POX 175)
- 0420-388 family. Only one strong line
- 0420-388 family. X,2,X,X,X at 5046 Å
- 0420-388 family. Helium discontinuity at 3700±30 Å
1321+294 (TON 157)
- z=0.960, group 15
1331+170
- z=2.081, group 30
- Identification of 3889 Å He II shell star absorption line
- 3389 Å (He I, Shell)
- Contains more than 10 absorption lines
1333+286 (RS 23)
- RS 23, PHL 1222, 1548+115b group
- z=1.908, group 26
1334+119
- z=1.760, group 23
1336+264 (RS 32)
- 3748 Å O II Wolf-Rayet laser line
1340+606 (3CR 288.1)
- z=0.961, group 15
1355-416
- z=0.313, group 3
1416+067 (3CR 298)
- z=1.439, group 50
- ROSAT (Jan 12 1993, 8884 sec., rp700865a01) 14 19 7.20 +06 28 48.0
- ROSAT (Jul 25 1992, 10714 sec., rp700865)
1422+202 (4C 20.33)
- z=0.871, group 41
1424-118
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1425+267 (TON 202)
- Significant proper motion, 0.05 arcsec/yr
- ROSAT (Jul 18 1993, 6716 sec., rp701369n00) 14 27 36.00 +26 32 24.0
- NRAO Images from the radio universe cd2:qsos/1425p267.
1442+101 (OQ 172)
- Contains more than 10 absorption lines and 3934 Ca II
- ROSAT (Aug 7 1992, 15433 sec., rp701002) 14 45 16.80 9 58 48.00
- VLBA Taylor
1448-232
- 0237-233 family.
- 0237-233 family. Emission lines 1,2,3,4,X,6 at 3900, 3980, 4480, 4970 and 6125 Å
1454-060
- z=1.249, group 48
1458+718 (3CR 309.1)
- z=0.908, group 14
- 3640, 5337
- ROSAT (Nov 27 1991, 9917 sec., p700330) 14 59 07.20 71 40 12.00
- VLBA Aaron
1502+602 (3C 311)
- z=1.022, group 16
1508-055
- z=1.191, group 19
- 4185, 3396 Å
1510-089
- z=0.361, group 35
- ROSAT (Aug 17 1992, 5153 sec., rp700854) 15 12 50.40 - 9 6 0.00
- VLBA Marscher 10/15/95
1512+132
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1512+370 (4C 37.43)
- Population inversion in 4686 Å He II
- z=0.370, group 4
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
- ROSAT (Aug 19 1992, 5230 sec., rp700807) 15 14 43.20 36 50 60.00
- NRAO Images from the radio universe cd2:qsos/1512p370.
1517+239 (LB 9612)
- z=1.901, group 26
1523+214 (LB 9707)
- Proper motion of 22.1±18 milliarcsec/yr
- z=1.924, group 55
1525+227 (LB 9743)
- z=0.253, group 32
1542+373 (4C 37.45)
- z=0.972, group 42
1545+210 (3CR 323.1)
- z=0.264, group 1
- ROSAT (Jan 19 1993, 3706 sec., rp700383n00) 15 47 43.20 +20 52 12.0
- NRAO Images from the radio universe cd2:qsos/1545p210.
- Near IR (K band, H band) nebulosity detected (Palomar 5.08 meter; Neugebauer,G., Matthews,K., Armus,L.: 1995, ApJ., 455, L123.)
1546+027
- z=0.412, group 6
1548+114
- RS 23, PHL 1222, 1548+115b group
- z=1.901, group 26
- Contains more than 10 absorption lines
- ROSAT (Jan 26 1993, 4048 sec., rp700386n00) 15 50 43.20 +11 21 0.0
1606+289 (4C 28.40)
- z=1.989, group 56
1607+183
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1611+343 (DA 406)
- z=1.401, group 20
- ROSAT (Aug 30 1992, 3651 sec., rp700842) 16 13 40.80 +34 12 36.0
- ROSAT (Jan 17 1993, 3153 sec., rp700842a01) 16 13 40.80 +34 12 36.0
- VLBA Beasley, Boboltz, Kemball, Lestrade, Romney
1623+269 (4C 26.48)
- z=0.779, group 39
1628+363 (4C 36.28)
- z=1.254, group 48
1634+269
- z=0.561, group 9
1638+398 (NRAO 512)
- VLBI Proper motion relative to 3C 345
- ROSAT (Sep 3 1992, 2857 sec., rp700843) 16 40 28.80 39 46 48.00
- VLBA Clark
1641+399 (3CR 345)
- double-lobes
- VLBI proper motion relative to NRAO 512
- Superluminal motion and Kellermann's paradoxes
- ROSAT (Jan 16 1992, 2604 sec., f700428) 16 41 16.80 39 54 00.00 2604
- ROSAT (Jan 16 1992, 3899 sec., p700428)
- ROSAT (Sep 1 1992, 4219 sec., rp700843) 16 42 57.60 39 48 36.00 4219 931018
- ROSAT (Mar 6 1993, 5986 sec., rp700870n00)
- ROSAT (Jul 19 1993, 1632 sec., rf700428a01) 16 41 16.00 +39 54 0.0
- ROSAT (Jul 19 1993, 946 sec., rp700428a01)
- VLBA Baath, Beasley, Claussen, Cornwell, Diamond, Kogan, Lobanov, Marcaide, Marvel, Romney, Weimer, Zensus
1657+265 (4C 26.51)
- Possibly 0420-388 family. Emission line at 5020 Å (He I 5015.7 or C IV 5018, 5017)
1702+298 (4C 29.50)
- z=1.927, group 55
1704+608 (3CR 351)
- z=0.371, group 4
- ROSAT (Oct 28 1991, 13068 sec., p700439) 17 04 40.80 60 44 24.00
- NRAO Images from the radio universe cd2:qsos/1704p608.
1741+279 (4C 27.38)
- z=0.372, group 4
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
1756+237
- Contains more than 10 absorption lines and 3934 Ca II
1801+010
- z=1.522, group 21
1816+475 (4C 47.48)
- 0237-233 family. Emission lines 1,X,3,4,X,X at 3928, 4508 and 4986 Å
2059+034
- Population inversion in 4686 Å He II
- z=0.370, group 4
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
2120+168 (3CR 432)
- 4349 Å O II Wolf-Rayet laser line
- z=1.805, group 24
2121+053 (OX 036)
- z=1.878, group 25
- VLBA Clark 08/31/95
2126-158
- Contains more than 10 absorption lines
- ROSAT (Nov 12 1992, 3968 sec., rp700868n00) 21 29 12.00 -15 39 0.0
- ROSAT (Apr 28 1993, 4160 sec., rp700868a01)
- ROSAT (May 9 1991, 3424 sec., rp700025)
- ROSAT (May 18 1993, 1610 sec., rp700025a01)
2145+067
- O VI sequence quasar
- 3811 and 3834 (O VI), 4658 (C IV), 4686 (He II)
- VLBA Aaron, Leppanen, Rupen
2149+212 (4C 21.59)
- z=1.534, group 51
2156+297 (4C 29.64)
- z=1.753, group 23
2201+315 (4C 31.63)
- z=0.297, group 2
- VLBA Leppanen 09/22/93
2223-052 (3C 446)
- z=1.404, group 20
- ROSAT (May 23 1993, 15626 sec., rp900337n00) 22 25 48.00 -04 57 0.0
2225-055 (PHL 5200)
- Identification of 3889 Å He II shell star absorption line
- 3389 Å (He I, Shell)
- P-Cygni emission lines observed in the optical spectra
- Mathur,S., Elvis,M., Singh,K.P.: 1995, ApJ., 455, L9. PHL 5200 ASCA X-Ray Spectra
2230+114 (CTA 102)
- z=1.037, group 17
- VLBA Leppanen, Marscher
2249+185 (3CR 454)
- z=1.757, group 23
2251+113
- z=0.323, group 33
- NRAO Images from the radio universe cd2:qsos/2251p113.
2251+158 (3CR 454.3)
- z=0.860, group 12
- ROSAT (Dec 16 1992, 22156 sec., rp900339n00) 22 53 57.60 +16 09 0.0
- ROSAT (May 27 1992, 8154 sec., rp700759) 22 53 57.60 16 8 60.00
- VLBA Bloom, Bower, Briggs, Clark, Claussen, Conway, Greenhill, Gwinn, Jowett, Kemball, Lestrade, Marscher, Pauliny-Toth, van Langev
- Kemball,A.J., Diamond,P.J., Pauliny-Toth,I.I.K.: 1996, ApJ., 464, L55. Continuum VLBA Polarimetry at 43 GHz. (taken on Dec 1, 1994)
- Pauliny-Toth,I.I.K., Porcas,R.W., Zensus,J.A., Kellermann,K.I., Wu,S.Y.: 1987, Nature, 328, 778. 'Superluminal' expansion during outburst (VLBI)
2251+244 (4C 24.61)
- Contains more than 10 absorption lines
2254+024
- z=2.090, group 31
2308+098 (4C 09.72)
- z=0.432, group 8
- NRAO Images from the radio universe cd2:qsos/2308p098
2320+079
- z=2.090, group 31
2325+269 (4C 27.52)
- z=0.875, group 41
2325+293 (4C 29.68)
- 3811+3834 (O VI), 4658 (C IV), 4686 (He II)
- O VI sequence quasar
2329-384
- z=1.195, group 19
- 4185, 3396 Å
2340-036
- z=0.896, group 13
2343+008
- 0805+046 family. Helium-rich shell star, 4713.14 He I emission
2346+385
- 2346+38; z=1.032, group 17
2351-154 (OZ 187)
- Contains more than 10 absorption lines
- ROSAT (Jun 16 1992, 6335 sec., wp701175) 23 54 31.20 -15 13 12.00
- ROSAT (12808 sec., wp701501n00) 23 54 28.00 -15 13 12.0
2353-685
- z=0.716, group 11
2353+283 (4C 28.59)
- z=0.731, group 38
2354+144
- z=1.810, group 24

Quasars are sorted by increasing RA (Right Ascension).

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