| Back to Interesting Follow-up Targets By: Sarah True |
This list of roughly 65 objects was completed circa 2009. It focuses on the excited troughs of HeI*, FeII*, FeIII*, NiII* and SiII*. Rolling over the object name will display a description for why the object was found interesting, and where applicable, how this object has been followed up.
NOTE: velocity is in units of 1000km/s (i.e. 2.4 is 2400km/s) and flux is in units of 10e-17 ergs/s/cm2/A.
| Object Name Comments | RA | Dec | File | U | g | r | I | z | Flux | Depth | Line | z | v | dv | Excited Troughs | Qual |
| J0149-1016 A few troughs from the 13.7k cm^-1 and 8.4k cm^-1 FeII* level detected; all 3 HeI* lines visible; Balmer lines of H* visible out to at least H-Delta; observed by us in Fall 2006 at Magellan/MIKE | 01 49 06.73 | -10 16 49.43 | 52174-0664-045 | 18.88 | 18.41 | 18.17 | 18.22 | 17.45 | 15 | 7 | FeII* | 0.36 | 1 | 0.3 | HeI* FeII* | D |
| J0318-0600 About 6 different systems; highly reddened QSO; SiII/SiII* 1808/1817 identified; a few NiII* transitions from 8k cm^-1 level; several FeII* from fine-structure of ground state; observed by us Fall 2006 VLT/UVES | 03 18 56.616 | -06 00 37.67 | 51924-0460-327 | 21.74 | 19.3 | 17.63 | 17.21 | 16.8 | 18 | 13 | FeII* | 1.93 | 1.1 | 0.5 | FeII* NiII* SiII* | D |
| J0745+1818 Wide blended troughs and only a few distinct well-separated lines; only 2 of 3 FeIII* present; FeII* and NiII* up to 8.4k cm^-1 but most are shallow and blended; ~2” away from a star of similar magnitude. | 07 45 54.741 | +18 18 17.03 | 52939-1582-256 | 19.94 | 19.41 | 18.76 | 18.67 | 18.52 | 11 | 4 | FeIII* | 1.06 | 2.3 | 1 | HeI* FeII* FeIII* NiII* | B |
| J0802+5513 Only HeI* 3890 visible; a couple of excited states of FeII resonance lines possibly present; CaII present; negative velocity so probably an infalling molecular cloud. | 08 02 48.19 | +55 13 28.94 | 53384-1871-440 | 20.84 | 19.23 | 18.44 | 17.91 | 17.7 | 8 | 4 | FeII* | 0.66 | -0.2 | 0.4 | HeI* FeII* | C |
| J0809+1818 Dozens of finely separated FeII* and NiII* lines!; FeII* has energies going up to 13k cm^-1 and possibly up to 27k cm^-1; NiII* goes up to 10K cm^-1. | 08 09 57.391 | +18 18 04.43 | 53319-1923-023 | 18.64 | 18.08 | 17.48 | 17.44 | 17.27 | 28 | 21 | FeII* | 0.97 | 2.1 | 0.7 | FeII* NiII* | A |
| J0822+2311 Shallow troughs of FeII* of fine-structure of ground state; possible identification of FeII* from 8K cm^-1 energies; all 3 HeI* barely detected; two unique systems in HeI* and MgII – possibly line locked with Mg II | 08 22 31.531 | +23 11 52.09 | 53317-1926-546 | 18.46 | 17.94 | 17.69 | 17.53 | 17.5 | 28 | 10 | FeII* | 0.65 | 0.6 | 0.5 | HeI* FeII* | A |
| J0835+4242 FeII* from fine-structure of ground state nicely separated; high column density because CaII present; all 3 HeI* lines present. | 08 35 22.775 | +42 42 58.29 | 52232-0762-085 | 18.67 | 18 | 17.64 | 17.49 | 17.22 | 24 | 10 | FeII* | 0.81 | 0.9 | 0.6 | HeI* FeII* | A |
| J0838+2955 Only SiII/SiII* 1527/1533 visible and is 1:1; possibly contaminated by CIV. | 08 38m17.01s | 29 55 26.56 | 52937-1269-277 | 18.71 | 18.3 | 17.85 | 17.6 | 17.43 | 20 | 5 | SiII* | 2.04 | 5.4 | 0.5 | SiII* | B |
| J0839+0454 SiII/SiII* 1260/1265 and 1527/1533 both present and deep; low velocity. | 08 39m26.616s | +04 54 20.29 | 52650-1188-390 | 21.55 | 20.23 | 18.77 | 18.37 | 18.17 | 5 | 4 | SiII* | 2.45 | 0.5 | 0.8 | SiII* | C |
| J0839+3805 SiII/SiII* 1527/1533 and 1808/1817 deep; all 3 FeIII* from 30.1 deep; dozens of troughs from FeII* up to 33.0k cm^-1 and NiII* up to 15.0k cm^-1 but many are wide and blended; only a few distinct uncontaminated transitions. | 08 39m42.114s | +38 05 26.42 | 52317-0828-007 | 21.61 | 19.61 | 18.94 | 18.95 | 18.61 | 9 | 7 | FeIII* | 2.32 | 0.6 | 1 | FeII* FeIII* NiII* SiII* | B |
| J0840+3633 Wide, blended troughs; SiII/SiII* 1808/1817 present but 1808 contaminated; FeII* lines up to 8k cm^-1 energy level; NiII* lines up to 10K cm^-1 energy; observed by de Kool et. Al (2002 ApJ 570 514) | 08 40 44.418 | +36 33 27.86 | 52320-0864-149 | 18.18 | 17.24 | 16.6 | 16.23 | 16.11 | 55 | 45 | FeII* | 1.23 | 0.8 | 1.1 | FeII* NiII* SiII* | D |
| J0859+4239 Extremely wide troughs; only a few distinct lines including: -SiII/SiII* 1808/1817 -the 3 FeIII* transitions of 30.1k cm^-1 - FeII* up to 27 cm^-1 and NiII* up to 15k cm^-1; all transitions between 2200 and 2800 in rest frame is blended. | 08 59 10.393 | +42 39 11.23 | 52294-0831-228 | 19.92 | 19.27 | 19.34 | 18.37 | 18.02 | 12 | 7 | FeIII* | 1.5 | 1.3 | 1.3 | FeII* FeIII* NiII* SiII* | B |
| J0922+0843 Dozens of distinct lines of FeII* up to 27.3k cm^-1 and NiII* up to 15.0k cm^-1 but ground terms and their excited states blended; all 3 FeIII* deep but only from 30.1k cm^-1 level; SiII/SiII* 1808/1817 present | 09 22 21.251 | +08 43 12.93 | 52763-1302-192 | 19.94 | 19.39 | 18.85 | 18.65 | 18.05 | 13 | 8 | FeIII* | 1.97 | 3.6 | 0.8 | FeII* FeIII* NiII* SiII* | A |
| J0929+2627 Only SiII/SiII* 1527/1533 present and appears 1:1 | 09 29 38.005 | +26 27 53.47 | 53383-1940-059 | 21.73 | 20.42 | 19.27 | 18.95 | 15.8 | 3 | 2 | SiII* | 2.25 | 3.9 | 0.8 | SiII* | C |
| J0932+0840 SiII/SiII* 1808/1817 present and deep; several distinct lines of NiII* up to 15k cm^-1; only excited states of ground term of FeII* present but mostly blended | 09 32 24.496 | +08 40 08.06 | 52993-1304-270 | 22.79 | 20.38 | 19.11 | 18.83 | 18.43 | 5 | 4 | SiII* | 2.3 | 0.5 | 0.4 | FeII* NiII* SiII* | B |
| J0933+3133 SiII/SiII* 1260/1265 and 1808/1817 present but 1:1; only the first 2 of 3 FeIII* lines from 30.1k cm^-1 level definitely present | 09 33 48.376 | +31 33 35.30 | 53386-1943-306 | 21.79 | 19.85 | 19.26 | 18.81 | 18.33 | 6 | 3 | SiII* | 2.6 | 2.4 | 0.7 | FeIII* SiII* | C |
| J0943+3243 Several distinct lines of FeII* from 1 up to 21k cm^-1 level to the right oc CIV; several NiII* up to 8.4 cm^-1; at least two systems and both contain all 3 FeIII* from the 30.1k cm^-1 level and the SiII/SiII* 1808/1818; in fact the two system look line locked with SiII/SiII* and/or FeIII* | 09 43 47.223 | +32 43 14.26 | 53387-1945-293 | 23.09 | 20.39 | 18.85 | 18.07 | 18.15 | 10 | 7 | FeIII* | 2.86 | 1.5 | 0.8 | FeII* FeIII* NiII* SiII* | B |
| J0957+4406 All 3 FeIII* from both 30k and 41k cm^-1 present; SiII/SiII* 1808/1817 is 1:1; FeII* up to 30k cm^-1 and NiII* up to 23k cm^-1 and up to 7 units deep! | 09 57 21.372 | +44 06 42.91 | 52703-0942-187 | 18.77 | 18.19 | 17.96 | 17.49 | 17.39 | 20 | 10 | FeIII* | 1.49 | 5.9 | 0.8 | HeI* FeII* FeIII* NiII* SiII* | A |
| J0957+5120 All 6 FeIII* from the 30.1k and 41.0k cm^-1 deep and wide especially the 30.1k cm^-1 levels; hints of FeII* and NiII* up to 8.4k cm^-1 although shallow at only 1-2 units deep and somewhat blended; appears to be two distinct systems with lower velocity component containing the excited lines. | 09 57 12.631 | +51 20 58.95 | 52409-0902-592 | 19.84 | 19.36 | 18.83 | 18.51 | 18.33 | 9 | 5 | FeIII* | 2.1 | 2.9 | 1.1 | FeII* FeIII* NiII* | B |
| J1002+3424 SiII/SiII* 1527/1533 present and 1527 is deeper so exact density can be constrained; excited states of FeII resonance possibly present; Unfortunately the absorber has low velocity so probably molecular cloud instead of outflow | 10 02 09.452 | +34 24 16.97 | 53388-1948-623 | 19.46 | 18.9 | 18.37 | 17.8 | 17.38 | 13 | 7 | SiII* | 1.92 | 0.2 | 0.4 | FeII* SiII* | C |
| J1006+0513 Many transitions of NiII* up to 15.0k cm^-1 and FeII* up to 27.3k cm^-1 but most are blended and contaminated; only a few distinct but shallow troughs | 10 06 05.665 | +05 13 49.02 | 52641-0996-243 | 20.11 | 19.45 | 18.87 | 18.62 | 18.27 | 7 | 3 | FeII* | 0.97 | 2.2 | 0.5 | FeII* NiII* | C |
| J1011+5155 Several distinct lines of FeII* from ground terms and NiII* up to 8.4k cm^-1; SiII 1808 present but not SiII* 1817; possibly up to 6 distinct systems | 10 11 08.895 | +51 55 53.82 | 52400-0903-068 | 22.41 | 20.61 | 18.83 | 18.13 | 17.77 | 8 | 4 | FeII* | 2.47 | 2.3 | 0.4 | FeII* NiII* | B |
| J1020+6023 Several lines of FeII* up to 13.7k cm^-1 and NiII* up to 8.4k cm^-1; only a few not blended; CaII and HI* possibly present but in a different slower system | 10 20 36.108 | +60 23 38.95 | 52370-0771-011 | 20.7 | 19.97 | 18.65 | 18.32 | 17.92 | 7 | 4 | FeII* | 0.99 | 1 | 0.6 | FeII* NiII* | B |
| J1021+0516 Only SiII/SiII* 1260/1265 present and 1265 could be contamination from atmospheric OI | 10 21 54.016 | +05 46 46.39 | 52319-0575-410 | 24.65 | 20.85 | 19.21 | 18.27 | 17.93 | 9 | 5 | SiII* | 3.47 | 4.5 | 1.1 | SiII* | B |
| J1022+3722 Dozens of transitions of FeII* up to 31k cm^-1 and NiII* up to 15k cm^-1 with transitions 8.4k cm^-1 and lower especially deep; several lines are blended but many distinct troughs exist; possible partial covering; SiII/SiII* 1808/1817 present but shallow; several transitions of FeII* shortward of AlIII exist | 10 22 36.229 | +37 22 41.44 | 53415-1957-390 | 21.52 | 19.91 | 18.9 | 18.33 | 17.77 | 7 | 5 | FeII* | 1.88 | 1.6 | 0.5 | FeII* NiII* SiII* | B |
| J1023+5005 Dozens of FeII* lines up to 8.4k cm^-1 level; a few NiII* from the 8.4k cm^-1 level; all 3 FeIII* from 30.1k cm^-1 level present. | 10 23 22.804 | +50 05 00.87 | 52707-1008-124 | 19.79 | 19.13 | 18.58 | 18.28 | 18.24 | 13 | 7 | FeIII* | 1.59 | 0.8 | 0.5 | Fe II* FeIII* NiII* | B |
| J1024+5553 Only the pair SiII/SiII* 1527/1533 visible | 10 24 37.427 | +55 53 01.27 | 52411-0947-243 | 20.18 | 19.67 | 19.2 | 18.9 | 18.79 | 5 | 2 | SiII* | 1.96 | 3.5 | 0.5 | SiII* | C |
| J1044+3656 Two outflows at 600 and 3400 km/s; the slower outflow has FeII* fine-structure of the ground state while the faster outflow has HeI* 3890 and CaII; possibly line locked in CaII; observed by de Kool et. Al (2001 ApJ 548 609) | 10 44 59.608 | +36 56 05.19 | 53463-2090-329 | 17.86 | 17.11 | 16.82 | 16.66 | 16.59 | 54 | 18 | FeII* | 0.7 | 0.6 | 0.7 | HeI* FeII* | D |
| J1050+0715 SiII/SiII* 1527/1533 present and 1:1; FeII present but no FeII*; low velocity | 10 50 49.735 | +07 15 54.82 | 52670-1001-502 | 19.96 | 19.44 | 18.95 | 18.62 | 18.41 | 9 | 4 | SiII* | 1.91 | 0.1 | 0.4 | SiII* | C |
| J1125+0029 Dozens of distinct troughs of FeII* up to 31k cm^-1 and NiII* up to 25k cm^-1; all 3 HeI* present; Hdelta present. | 11 25 26.125 | +00 29 01.32 | 51614-0281-427 | 19.46 | 19.32 | 18.33 | 18.05 | 17.83 | 14 | 6 | FeII* | 0.86 | 0.8 | 0.4 | HeI* FeII* NiII* | B |
| J1127+4859 SiII/SiII* 1527/1533 and 1808/1817 present; a few lines of NiII* up to 8.4k cm^-1 and FeII* from the ground term | 11 27 36.705 | +48 59 39.30 | 52642-0966-274 | 21.28 | 19.71 | 18.65 | 18.25 | 18.19 | 6 | 5 | SiII* | 1.83 | 1.6 | 0.6 | FeII* NiII* SiII* | B |
| J1128+0113 Several distinct lines of FeII* up to 27.3k cm^-1 and NiII* up to 15.0k cm^-1; resonance lines and excited lines of ground state blended however | 11 28 28.315 | +01 13 37.97 | 51992-0512-123 | 19.74 | 19.56 | 18.6 | 18.35 | 18.02 | 9 | 6 | FeII* | 0.89 | 1.6 | 0.4 | FeII* NiII* | B |
| J1130+0411 SiII/SiII* 1527/1533 and 1808/1817 present and 1806 appears deeper than 1817; several low energy FeII* transitions up to 3k cm^-1 longward of CIV; several narrow and distinct transitions of ground NiII | 11 30 10.58 | +04 11 28.05 | 52642-0837-220 | 24.12 | 22.21 | 19.3 | 18.09 | 17.4 | 10 | 10 | SiII* | 3.93 | 0.5 | 0.9 | FeII* SiII* | A |
| J1134+3238 Highly blended but several distinct lines of FeII* up to 13.7k cm^-1 and NiII* up to 9.3k cm^-1; SiII/SiII* 1808/1817 present; several unidentified lines between 2000 and 2300 in the rest frame of the QSO which are probably ground state transitions of Mg I, Cr II and/or Cu II | 11 34 24.642 | +32 38 02.45 | 53460-2098-251 | 22.67 | 20.63 | 18.55 | 18.05 | 17.4 | 12 | 9 | FeII* | 2.46 | 2.8 | 0.9 | FeII* NiII* SiII* | A |
| J1138+4001 All 3 lines of HeI* visible; two transitions of FeII* from 13.5/13.7k cm^-1 detected; low velocity | 11 38 04.885 | +40 01 18.95 | 53466-1972-484 | 19.76 | 19.01 | 18.24 | 18.16 | 17.37 | 10 | 2 | FeII* | 0.29 | 0.2 | 0.5 | HeI* FeII* | C |
| J1145+1100 Dozens of deep distinct transitions of FeII* up to 26k cm^-1 and NiII* up to 15k cm^-1; unfortunately low velocity | 11 45 56.25 | +11 00 18.44 | 52734-1266-375 | 19.91 | 19.3 | 18.94 | 18.8 | 18.52 | 8 | 7 | FeII* | 0.93 | 0.2 | 0.3 | HeI* FeII* NiII* | C |
| J1206+0023 Very shallow and noisy troughs of FeII* definitely up to 13.7k cm^-1 and possibly up to 27k cm^-1; only a few well defined non-blended transitions | 12 06 27.623 | +00 23 35.54 | 51999-0286-499 | 20.91 | 20.19 | 19.07 | 18.68 | 18.55 | 4 | 3 | FeII* | 1.11 | 1.9 | 0.4 | HeI* FeII* | C |
| J1211+1438 Only HeI* 3890 visible; a couple of excited states of FeII resonance lines possibly present but blended/noisy; slow velocity so probably a molecular cloud. | 12 11 18.669 | +14 38 10.46 | 53466-1765-197 | 19.13 | 18.56 | 18.48 | 18.21 | 18.45 | 11 | 3 | FeII* | 0.58 | 0.2 | 0.5 | HeI* FeII* | C |
| J1215+4406 Only SiII/SiII* 1260/1265 present and appears near 1:1 | 12 15 00.374 | +44 06 30.14 | 53090-1370-119 | 22.83 | 19.57 | 19.24 | 18.76 | 18.51 | 10 | 7 | SiII* | 2.91 | 1 | 0.8 | SiII* | B |
| J1219+6725 All 3 FeII* from 30k cm^-1 present but shallow | 12 19 44.000 | +67 24 05.92 | 51957-0493-593 | 18.75 | 18.31 | 17.99 | 17.83 | 17.87 | 22 | 5 | FeIII* | 1.57 | 3.9 | 0.4 | FeIII* | B |
| J1224+3632 All 3 FeIII* from 30k cm^-1 present; 3 distinct systems; SiII/SiII* 1527/1533 and 1808/1817 present and 1:1; FeII* has separated lines from fine structure of ground state: several 2-3k cm^-1 right of CIV absorption and energies up to 27k cm^-1 – all fairly shallow with depths of 4-5; NiII* up to 15k cm^-1 | 12 24 07.54 | +36 32 24.18 | 53442-2003-497 | 19.12 | 18.45 | 17.89 | 17.45 | 17.26 | 19 | 9 | FeIII* | 1.76 | 2 | 0.6 | HeI* FeII* FeIII* NiII* SiII* | A |
| J1226+1209 All 3 HeI* present and 3-9 units deep; FeII* up to 13.7k cm^-1 present and separated longward of MgII but blended/noisy shortward of MgII | 12 26 14.971 | +12 09 25.41 | 53120-1614-145 | 19.41 | 19.02 | 18.21 | 18.1 | 17.88 | 14 | 2 | FeII* | 0.87 | 1.1 | 0.3 | HeI* FeII* | C |
| J1227+5053 A few shallow lines of FeII* from the ground term present; HeI* fairly deep; CaII present | 12 27 03.19 | +50 53 56.30 | 52644-0971-459 | 21.08 | 19.44 | 18.54 | 18.09 | 17.66 | 6 | 3 | FeII* | 0.76 | 1.3 | 0.3 | HeI* FeII* | C |
| J1259+1213 Extremely wide and blended troughs; possibly a few distinct FeII* from the 13.7k cm^-1 level detected; all 3 HeI* lines present; HI* down to at least H-delta | 12 59 42.803 | +12 13 12.60 | 53473-1695-075 | 19.83 | 19.21 | 18.51 | 18.19 | 18.08 | 10 | 3 | FeII* | 0.75 | 2.5 | 1.3 | HeI* FeII* | C |
| J1319+0550 Dozens of distinct transitions of FeII* up to 32.9k cm^-1 and NiII* up to 15k cm^-1; the 3 FeIII* 30.1k cm^-1 transitions present; HeI* 3189 and 3890 visible | 13 19 50.446 | +05 50 44.85 | 52376-0851-524 | 20.33 | 19.9 | 19.23 | 18.96 | 16.79 | 4 | 3 | FeII* | 1.06 | 0.8 | 0.5 | HeI* FeII* FeIII* NiII* | C |
| J1319+2833 SiII//SiII* 1808/1817 present but 1:1; FeIII* from 30k and 41k cm^-1 energy levels detected; all FeII* and NiII* beyond 2100 AA in rest frame blended | 13 19 57.704 | +28 33 11.11 | 53471-2002-136 | 19.06 | 18.45 | 17.61 | 17.21 | 16.79 | 21 | 12 | FeIII* | 2.04 | 4.4 | 1.3 | FeII* FeIII* NiII* SiII* | A |
| J1321-0041 SiII/SiII* 1808/1817 distinct while other SiII/SiII* pairs blended; 3 transitions of FeIII* shallow but present; a few NiII* up to 8.4k cm^-1; too high redshift to see any FeII* | 13 21 57.704 | -00 41 52.04 | 51984-0296-153 | 23.7 | 20.45 | 19.25 | 18.64 | 18.39 | 5 | 3 | SiII* | 3.07 | 2 | 0.7 | FeIII* NiII* SiII* | C |
| J1333+4556 Dozens of distinct narrow transitions of FeII* (including lower energies to the right of CIV) up to 20k cm^-1 and NiII* up to 15k cm^-1; unfortunately atmospheric noise dominate beyond 8500 AA; SiII/SiII* 1260/1265 1304/1309 1527/1533 and 1808/1817 present; all 3 FeIII* from 30.1k cm^-1 visible. | 13 33 32.732 | +45 56 06.22 | 53063-1463-075 | 21.16 | 19.45 | 19.18 | 18.87 | 18.57 | 7 | 4 | SiII* | 2.64 | 1.8 | 0.5 | FeII* FeIII* NiII* SiII* | B |
| J1334+3205 A few distinct FeII* transitions from the ground term visible in the 2383 group but not in the 2600 group; only HeI* 3890 visible | 13 34 41.591 | +32 05 54.65 | 53468-2109-170 | 20.02 | 19.39 | 19.13 | 19.05 | 18.88 | 8 | 5 | FeII* | 0.67 | 0.7 | 0.3 | HeI* FeII* | B |
| J1341-0036 FeII* and NiII* up to 20.3k cm^-1 and 10.7k cm^-1 respectively but shallow troughs of ~2-3 units; many distinct transitions including several FeII* right of EVI emission; all 3 FeIII* from 30.1k cm^-1 visible; all SiII/SiII* (1260 1304 1527 1808/1265 1309 1533 1817) present | 13 41 45.128 | -00 36 31.21 | 51671-0299-172 | 20.88 | 19.66 | 19.01 | 18.52 | 18.27 | 8 | 4 | FeIII* | 2.22 | 2.4 | 0.5 | FeII* FeIII* NiII* SiII* | B |
| J1352+4239 Highly blended troughs – there are no distinct transitions of FeII*; the only possible distinct excited transiton is the SiII/SiII* 1808/1817 | 13 52 46.373 | +42 39 23.58 | 52814-1345-027 | 20.79 | 18.65 | 17.53 | 17.69 | 16.48 | 16 | 3 | SiII* | 2.04 | 9.5 | 1.6 | FeII* SiII* | C |
| J1439-0106 SiII/SiII* 1527/1533 visible and 1527 is deeper so exact densities can be constrained; a few transitions of FeII* from the ground term visible | 14 39 07.511 | -01 06 16.76 | 52409-0919-566 | 19.74 | 19.3 | 18.98 | 18.59 | 18.39 | 10 | 6 | SiII* | 1.82 | 2.4 | 0.3 | FeII* SiII* | B |
| J1440+3710 Several lines of NiII* and FeII* lines up to 8.4k cm^-1; many transitions near ground term of FeII blended but a few well-separated distinct lines | 14 40 02.245 | +37 10 58.52 | 53115-1382-482 | 23.03 | 20.32 | 18.99 | 18.06 | 17.74 | 7 | 5 | FeII* | 1.41 | 3.4 | 0.4 | FeII* NiII* | B |
| J1448+4043 Highly blended troughs; FeII* possibly up to 8k cm^-1 and NiII* possibly up to 10k cm^-1; low velocity | 14 48 00.146 | +40 43 11.72 | 53119-1397-198 | 19.98 | 18.5 | 17.08 | 16.78 | 16.47 | 28 | 9 | FeII* | 0.8 | 0.1 | 0.7 | FeII* NiII* | C |
| J1508+6055 Several lines of FeII* from excited states of ground terms and NiII* up to 8.4k cm^-1; unfortunately many contaminated by a second intervening system | 15 08 48.798 | +60 55 51.90 | 52055-0611-114 | 21.46 | 19.57 | 18.65 | 17.54 | 17.45 | 9 | 4 | FeII* | 1.53 | 3.7 | 0.8 | FeII* NiII* | B |
| J1620+4157 Wide blended troughs of the FeIII* from 30.1k cm^-1 FeII* up to 27.3k cm^-1 and NiII* up to 15.0k cm^-1; only a few distinct uncontaminated troughs | 16 20 16.604 | +41 57 44.14 | 52753-1171-603 | 19.75 | 19.35 | 18.9 | 18.65 | 18.58 | 9 | 3 | FeIII* | 1.29 | 1.8 | 0.8 | HeI* FeII FeIII* NiII* | C |
| J1624+3538 SiII/SiII* 1527/1533 and 1808/1817 present and the ground state deeper so exact densities can be constrained; probably molecular cloud since infalling | 16 24 19.962 | +35 38 45.28 | 52522-1057-612 | 19.59 | 18.75 | 18.21 | 17.78 | 17.55 | 13 | 7 | SiII* | 1.77 | -0.5 | 0.6 | SiII* | C |
| J1634+4640 SiII//SiII* 1527/1533 deep; several distinct lines of FeII* from the ground term and 8.4k cm^-1 level but very shallow with depths of 1-2 units; CIV is offset about 300 km/s slower than the other transitions of the same system – interesting | 16 34 31.805 | +46 40 37.01 | 52144-0627-172 | 19.26 | 19.2 | 19.09 | 18.73 | 18.67 | 13 | 5 | SiII* | 1.83 | 0.7 | 0.4 | FeII* SiII* | B |
| J1718+2643 Only the pair SiII/SiII* 1260/1265 distinctly visible and deep; SiII/SiII* 1527/1533 possibly present but contaminated by CIV | 17 18 13.250 | +26 43 52.20 | 52427-0979-185 | 20.22 | 18.65 | 19.19 | 18.85 | 18.6 | 8 | 5 | SiII* | 2.08 | 2.2 | 0.7 | SiII* | B |
| J1723+5553 Dozens of distinct troughs of FeII* up to 31k cm^-1 and NiII* up to 25k cm^-1; all 3 FeIII* lines from 30.1k cm^-1 are deep | 17 23 41.089 | +55 53 40.57 | 51997-0367-506 | 20.54 | 20.14 | 18.36 | 18.52 | 17.65 | 16 | 10 | FeIII* | 2.13 | 2.4 | 0.7 | FeII* FeIII* NiII* SiII* | A |
| J2107-0620 Hundreds of FeII* transitions up to energies 30k cm^-1; many of them are well separated!!!; observed by Pat Hall 2005 VLT/UVES and us Fall2006 Magellan/MIKE | 21 07 57.664 | -06 20 10.63 | 52174-0637-610 | 18.21 | 17.49 | 17.23 | 16.84 | 16.78 | 39 | 20 | FeII* | 0.65 | 1.2 | 0.6 | HeI* FeII* NiII* | D |
| J2151+0053 SiII/SiII* 1527/1533 and SiII 1808 visible; SiII 1527 deeper than SiII* 1533 so exact densities can be constrained; low velocity so probably molecular cloud | 21 51 51.606 | +00 53 23.17 | 52078-0371-452 | 19.17 | 18.75 | 18.53 | 18.18 | 18.13 | 19 | 6 | SiII* | 1.83 | 0.2 | 0.5 | SiII* | C |
| J2226+1427 Dozens of distinct separated lines of FeII* from ground terms and up to 8.0k cm^-1; a few NiII* from 8.4k cm^-1; SiII* 1533 also present; observed by us Fall 2006 with Magellan/MIKE | 22 26 16.501 | +14 27 14.65 | 52518-0737-523 | 20.02 | 19.39 | 18.89 | 18.48 | 18.38 | 8 | 6 | FeII* | 1.67 | 1.1 | 0.4 | FeII* NiII* SiII* | D |
| J2305+1517 All 3 FeIII* 30k cm^-1 and HeI* identified with troughs having depths of 11 and 7 respectively; unfortunately SiII* 1817 FeII* up to 27k cm^-1 and NiII* up to 15k cm^-1 are shallow at depths ~4; all 3 FeIII* 40k cm^-1 are also present; H-delta quite visible; QSO is 6.4' away from 2.5 mag star- alpha Peg, Markab | 23 05 01.003 | +15 17 34.99 | 52262-0743-337 | 18.73 | 18.18 | 17.73 | 17.56 | 17.43 | 18 | 11 | FeIII* | 1.12 | 1.1 | 0.7 | HeI* FeII* FeIII* NiII* SiII* | B |
| J2357-0048 SiII/SiII* 1260 1304 1527/1265 1309 1533 present but appear 1:1 | 23 57 02.549 | -00 48 24.00 | 51791-0387-246 | 21.9 | 19.47 | 19.03 | 18.73 | 18.52 | 9 | 5 | SiII* | 3.01 | 2.7 | 0.4 | SiII* | B |
Maintained by the Virginia Tech Quasar Outflow Group. Please cite responsibly.
