SDSS Search 2018: Part III Back to Interesting Follow-up Targets
By: Xinfeng Xu

This is a list of the interesting objects found with z > 2 with magnitude g < 18, epoch > 01/01/2011.

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
Objectfile nameredshiftRADecfluxdepthlineVdVgradeComments
SDSSJ1007+0532spSpec-55677-4875-328.fit2.88010:07:11.81+05:32:08.971501.10SiIV-4.70.7A+Has good SiIV & SiIV excited. Can be observed from VLT. Object is very bright about 10^-15. Strong seperated SiIV. Wrong Redshift
>1500 Dec
SDSSJ0831+5325spSpec-57012-7302-588.fit2.79408:31:04.90+53:25:00.15350.90SiIV-7.84.6A good SIV follow up. Has wide deep SiIV. Interesting but unobservable with VLT. Wrong Redshift
SDSSJ0845+3420spSpec-56337-5186-554.fit2.14508:45:38.66+34:20:43.62301.07SiIV-9.78.1Good northern hemisphere follow up target.
SDSSJ0916+6213spSpec-56722-7446-523.fit2.80709:16:10.33+62:13;26.69601.79SiIV-6.55.7Good northern hemisphere follow up target. Has good SiIV. Wrong Redshift.
SDSSJ1004+4700spSpec-56338-6663-220.fit2.53610:04:59.14+47:00:58.00380.92CIV-196.6CIV system at around 25000km/s. Interesting Object.
SDSSJ1029+6223spSpec-56667-7097-456.fit2.46610:29:00.79+62:23:42.16370.59CIV1.40.4Possible redshifted CIV
SDSSJ1107+6420spSpec-56746-7110-476.fit2.30711:07:35.57+64:20:09.07680.22CIV2.40.2Possible redshifted CIV
SDSS1230+4014spSpec-55704-3967-872.fit2.04712:30:11.84+40:14:42.92621.44CIV-2.00.5Interesting since we see SiII&SiII* and CII&CII*
SDSSJ1623+4818 spSpec-56448-6317-445.fit2.850 16:23:31.15 +48:18:42.29 300.57 SiIV-0.82 0.1 B+ Possible SIV & SIV* but looks too strong. Probable NIII & NIII*

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