| Back to Interesting Follow-up Targets By: Sarah True |
This is a list of all the interesting objects found with magnitude 18.2 < g < 18.7.
The names of each object are linked to the PDF of the SDSS spectra with the ions of each system identified. The blue system is considered the "main" system. Multiple PDFs of the same object indicate a different main system for each.
* indicates a blended trough (and therefore less accurate velocity calculations)
NOTE: Velocity is in units of 1000km/s. (e.g. 2.4 = 2400km/s) and flux is in units of 10e-17 ergs/s/cm2/A.
| Object | file name | Redshift | RA | Dec | flux | depth | line | V | dV | grade | Comments |
| SDSSJ0046+0104 | spSpec-51794-0393-572.fit | 2.152 | 00 46 13.536 | +01 04 25.74 | 38 | 5 | SiIV | -2 | 0.34 | A | very deep SiIV @ 2000km/s, shallower system @ 12000km/s, redshift correction? |
| SDSSJ0200-0037 | spSpec-51871-0403-070.fit | 2.141 | 02 00 06.308 | -00 37 09.91 | 15 | 1 | SiIV | -8.5 | 1.3 | A | Strong, wide SiIV @ 8500km/s |
| SDSSJ0242+0049 | spSpec-51821-0408-576.fit | 2.069 | 02 42 21.864 | +00 49 12.7 | 23 | 1 | SiIV | -2.6 | 0.78 | A | strong, narrow SiIV; SiII and SiII*; CII and CII*, good redshift based on MgII |
| SDSSJ0805+1219 | spSpec-53794-2418-521.fit | 2.336 | 08 05 20.559 | +12 19 54.85 | 22 | 8 | SiIV | 1.6 | 0.45 | A- | remote possibility of CII* infall, |
| SDSSJ0825+0740 | spSpec-53084-1758-222.fit | 2.194 | 08 25 25.071 | +07 40 14.33 | 30 | 22 | SiIV | 1.4 | 0.23 | A- | Redshift based on very broad MgII, possible CII* infall |
| SDSSJ0831+0354 | spSpec-52646-1186-294.fit | 2.077 | 08 31 26.16 | +03 54 08.1 | 25 | 10 | SiIV | -11 | 1 | A+++ | 11,000 km/s outflow, deep wide SiIV |
| SDSSJ0910+5746 | spSpec-51907-0484-134.fit | 2.222 | 09 10 35.453 | +57 46 43.26 | 23 | 5 | SiIV | -2 | 1.1 | A+ | WHT, 2-3 strong SiIV troughs |
| SDSSJ0913+4420 (I) | spSpec-52312-0832-195.fit | 2.936 | 09 13 07.83 | +44 20 14.36 | 20 | 2 | SiIV | -3.3 | 1.4 | A | WHT, 2 main systems ~3000 km/s SIV*, 11,000 SIV/SIV* blended but possible PV. |
| SDSSJ0913+4420 (II) | spSpec-52312-0832-195.fit | 2.936 | 09 13 07.83 | +44 20 14.36 | 15 | 3 | SiIV | -11 | 1.6* | ||
| SDSSJ0929+0216 | spSpec-51965-0475-457.fit | 2.108 | 09 29 38.284 | +02 16 28.73 | 26 | 10 | SiIV | -2.5 | 0.28 | A- | narrow SiIV, possible CIII*? SIV? |
| SDSSJ0941+1331 | spSpec-54092-2580-598.fit | 2.021 | 09 41 11.118 | +13 31 31.2 | 34 | 10 | SiIV | -3.1 | 0.5 | A+ | 3 strong CIV troughs, only 1 strong narrow SiIV @ 3100km/s, possible SiII/SiII* |
| SDSSJ1016+1218 | spSpec-53061-1745-108.fit | 2.313 | 10 16 25.979 | +12 18 38.62 | 18 | 10 | SiIV | -12 | 2.2* | A | 2 strong CIV troughs, only 1 strong broad SiIV @ 12,000km/s |
| SDSSJ1054+2536 | spSpec-53793-2357-227.fit | 2.4 | 10 54 27.18 | +25 36 00.86 | 26 | 1 | SiIV | -3 | 1.2 | A+ | WHT, Deep wide SiIV with little blending, 3 CIV systems; Obs with HIRES in 1998 |
| SDSSJ1055+2702 | spSpec-53793-2357-413.fit | 2.141 | 10 55 31.439 | +27 02 25.89 | 20 | 5 | SiIV | -3 | 1 | A | WHT, 2 deep systems of SiIV, strong CII, AlIII |
| SDSSJ1111+1437 | spSpec-53377-1751-630.fit | 2.136 | 11 11 10.148 | +14 37 57.07 | 25 | 8 | SiIV | -1.5 | 0.34 | A- | only SiIV no other low ionization species, high ionization outflow |
| SDSSJ1122+1645 | spSpec-54176-2499-308.fit | 3.031 | 11 22 58.773 | +16 45 40.33 | 32 | 5 | SiIV | -12.4 | 8.1* | A | possible narrow SIV/SIV*, possible PV, possible strong damp Lya system |
| SDSSJ1124+5502 | spSpec-52707-1014-347.fit | 2.932 | 11 24 40.822 | +55 02 33.77 | 12 | 3 | SiIV | -2.8 | 0.44 | A | Possible NIII/NIII*, SiIV AOD |
| SDSSJ1133+1447 | spSpec-53385-1754-558.fit | 3.244 | 11 33 30.179 | +14 47 58.92 | 18 | 13 | SiIV | -2.9 | 0.51 | A+++ | NeVIII and OIV 790* accessible with VLT; SVI Lyb/Lya possible SIV/SIV* seen |
| SDSSJ1135+1615 | spSpec-53856-2503-138.fit | 2.004 | 11 35 12.697 | +16 15 50.65 | 28 | 5 | SiIV | -6.8 | 7.0* | A+ | high velocity, wide deep SiIV |
| SDSSJ1203+0524 | spSpec-52376-0842-425.fit | 2.123 | 12 03 26.312 | +05 24 45.73 | 20 | 13 | SiIV | -1.8 | 0.48 | A- | 2 narrow (~500km/s) SiIV components |
| SDSSJ1227+0212 | spSpec-52288-0520-306.fit | 2.134 | 12 27 18.08 | +02 12 25.55 | 22 | 15 | SiIV | -15.2 | 1.1 | A- | high velocity, shallow SiIV |
| SDSSJ1245+0105 | spSpec-51928-0291-612.fit | 2.809 | 12 45 51.445 | +01 05 5.04 | 15 | 10 | SiIV | -6 | 4.7 | A | SIV/SIV*, high redshift |
| SDSSJ1259+6212 | spSpec-52320-0782-151.fit | 3.24 | 12 59 03.263 | +62 12 11.69 | 17 | 4 | SiIV | -0.47 | 0.61 | C | low velocity, almost certainly an intervening system |
| SDSSJ1324+2452 (I) | spSpec-54524-2664-537.fit | 2.363 | 13 24 22.544 | +24 52 22.39 | 23 | 4 | SiIV | -5.4 | 1.1 | A | WHT, 2 strong SiIV @ 7.4 & 5.4 |
| SDSSJ1324+2452 (II) | spSpec-52524-2664-537.fit | 2.363 | 13 24 22.544 | +24 52 22.39 | |||||||
| SDSSJ1347+4654 (I) | spSpec-52736-1284-140.fit | 2.933 | 13 47 22.837 | +46 54 28.6 | 25 | 2 | SiIV | -2.5 | 1.7 | A | WHT, 2 strong SiIV @ 4 & 2.5 |
| SDSSJ1347+4654 (II) | spSpec-52736-1284-140.fit | 2.933 | 13 47 22.837 | +46 54 28.6 | |||||||
| SDSSJ1405+0229 | spSpec-51993-0532-429.fit | 2.808 | 14 05 32.904 | +02 29 57.32 | 15 | 5 | SiIV | -7.9 | 1 | A- | CIII*, small chance of SIV due to contamination of SIV* position |
| SDSSJ1413+0922 | spSpec-53794-1810-516.fit | 3.346 | 14 13 21.057 | +09 22 4.89 | 46 | 22 | SiIV | -34.4 | 0.5 | A- | 6 & 7 components CIV, high velocity is intervening, other systems need work before further observations. |
| SDSSJ1502-0240 | spSpec-52426-0922-258.fit | 2.215 | 15 02 05.581 | -02 40 38.56 | 25 | 10 | SiIV | -11.1 | 0.52 | A- | many blended systems makes ID hard. |
| SDSSJ1554+2218 | spSpec-53557-2171-479.fit | 2.414 | 15 54 33.131 | +22 18 42.08 | 21 | 1 | SiIV | -4.3 | 2.2 | A | WHT, deep and broad SiIV, possible CIII* and good chance for SIV* |
| SDSSJ2218-0834 | spSpec-52203-0719-588.fit | 2.539 | 22 18 38.218 | -08 34 50.05 | 18 | 12 | SiIV | -11 | 0.69 | A+ | 12,000 km/s outflow w/ possible CIII* (minus 8 dec and 2.5 redshift makes promising) |
| SDSSJ2257-1001 | spSpec-52254-0724-150.fit | 2.08 | 22 57 19.043 | -10 01 04.74 | 20 | 12 | CI | -24.8 | 0.3 | ?? | Intervening systems with CI small possibility of CI*, probably a damp Lya system. |
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