| Back to Interesting Follow-up Targets By: Xinfeng Xu |
This is a list of the interesting objects found with 0.5 < z < 2 with magnitude 17 < g < 18, all epochs.
The search was done by REU students: Sean Collier, Sean Heston, and Jake Pighini and was checked by Nahum Arav.
The names of each object are linked to the PDF file of the SDSS spectra with the ions of each system identified. The blue system is considered the "main" system.
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. If the rest wavelength of 1350 angstroms was not in the range, flux was identified at 1600 angstroms.
| <1500 Dec | |||||||||||
| Object | file name | redshift | RA | Dec | flux | depth | line | V | dV | grade | Comments |
| SDSSJ0412-0511 | spSpec-51910-465-603.fit | 0.550 | 04:12:10.18 | -05:11:09.26 | 55 | 0.17 | HeI* | -0.8 | 0.5 | Solid 3890 HeI*. | |
| SDSSJ1044+0518 | spSpec-55648-4773-908.fit | 0.905 | 10:44:30.26 | +05:18:57.29 | 40 | 0.34 | HeI* | -2.8 | 0.2 | Narrow HeI*. | |
| SDSSJ1054+1255 | spSpec-53358-1750-212.fit | 1.822 | 10:54:18.86 | +12:55:12.49 | 40 | 2.30 | SiIV | -3.7 | 0.7 | Low ionization BAL. | |
| SDSSJ1309+0119 | spSpec-52295-525-250.fit | 0.547 | 13:09:52.88 | +01:19:50.76 | 55 | 0.20 | HeI* | 0.0 | 0.2 | Definite HeI*. | |
| SDSSJ1532+0613 | spSpec-55735-4885-306.fit | 0.837 | 15:32:09.51 | +06:13:56.13 | 70 | 0.32 | HeI* | -3.0 | 0.6 | Strong HeI*. Possible FeII* 2396. | |
| SDSSJ2215-0045 | spSpec-55443-4201-464.fit | 1.474 | 22:15:11.94 | -00:45:50.00 | ~~ | 2.66 | CIV | -10.4 | 20 | Fe low BAL. | |
| >1500 Dec | |||||||||||
| SDSSJ0822+2311 | spSpec-53317-1926-546.fit | 0.653 | 08:22:31.53 | +23:11:52.09 | 35 | 0.38 | HeI* | -0.9 | 0.7 | Fe low BAL with excited troughs from UVI UVII and UVIII. Possible troughs from higher multiple. Strong HeI*. | |
| SDSSJ0826+4254 | spSpec-54524-761-414.fit | 0.709 | 08:26:04.66 | +42:54:35.85 | 50 | 0.19 | HeI* | -2.4 | 1.1 | Wide HeI* BAL. | |
| SDSSJ0832+5256 | spSpec-55925-5156-326.fit | 0.789 | 08:32:52.82 | +52:56:37.81 | 55 | 0.18 | HeI* | -3.0 | 0.4 | HeI* troughs present. | |
| SDSSJ1028+4500 | spSpec-56783-7388-362.fit | 0.584 | 10:28:39.11 | +45:00:09.43 | 50 | 0.47 | HeI* | -0.7 | 0.5 | Probable HeI*. | |
| SDSSJ1116+4345 | spSpec-56013-4686-594.fit | 0.801 | 11:16:28.00 | +43:45:05.85 | 50 | 0.274 | HeI* | -4.1 | 0.7 | HeI* has all three lines present and looks saturated. | |
| SDSSJ1239+1800 | spSPec-54243-2600-482.fit | 1.273 | 12:39:59.78 | +18:00:57.72 | 60 | 0.58 | HeI* | -1.9 | 0.5 | Strong HeI* lines and has all three. | |
| SDSSJ1242+6246 | spSpec-56444-6970-561.fit | 1.296 | 12:42:44.37 | +62:46:59.11 | 80 | 0.15 | FeII | -9.0 | 1.0 | Fe low BAL. Wide troughs. High excitation FeII absorption. | |
| SDSSJ1253+2934 | spSpec-54892-3236-166.fit | 1.762 | 12:53:12.38 | +29:34:16.78 | 35 | 1.53 | CIV | -12.7 | 1.3 | High velocity CIV outflow system. Also has two redshifted systems. | |
| SDSSJ1319+4222 | spSpec-53112-1461-371.fit | 0.642 | 13:19:56.82 | +42:22:08.32 | 60 | 0.13 | HeI* | -2.1 | 0.4 | Definite HeI* with all three lines visible. | |
| SDSSJ1429+5238 | spSpec-56448-7030-4.fit | 0.595 | 14:29:27.28 | +52:38:49.83 | 40 | 0.27 | HeI* | -4.1 | 0.6 | Wide HeI* system that looks saturated. | |
| SDSSJ1443+6332 | spSpec-56447-6983-678.fit | 1.401 | 14:43:58.61 | +63:32:26.42 | 55 | 0.19 | HeI* | -5.5 | 0.4 | FeII* in multiple UV. Also has HeI*. | |
| SDSSJ1508+3404 | spSpec-55691-4720-591.fit | 0.787 | 15:08:47.42 | +34:04:37.73 | 36 | 0.48 | HeI* | 0.7 | 0.8 | Very strong HeI*. | |
| SDSSJ1557+3120 | spSpec-55748-5010-728.fit | 0.792 | 15:57:00.39 | +31:20:20.12 | 60 | 0.22 | HeI* | -4.0 | 0.7 | Definite HeI*. | |
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