This is supposed to be a quasar star. Its chart is peaish.
I'm still not convinced that there isn't some formula stating that the OIII ( In my terms i think that means Triply ionised oxygen?) isn,t a certain percentage above the background.
These border line charts may tell us what processes are going on to go up to or come down from the supper high OIII? does anyone else think the same way? Sorry my chemistry stops at how much sugar to put in a cup of coffee. so I'm just guessing
This looks like a back to front chart
I don't fully understand z charts but Fermats Brother was saying that about .85 was the highest Z for a pea. The OIII seems at the wrong end of the chart
Maybe some one else understands? ( I,ve tried bashing my head against the wall it does't work for me, SIGH, LOL)
STAR ra=208.06983235, dec=2.7573619, ObjId = 587726033334567091
http://cas.sdss.org/astro/en/tools/explore/obj.asp?id=587726033334567091

Sorry if this doesn't make sense. I think like a marble in a bucket. LOL