Emission Lines in High Redshift QSOS

Details Emission Lines in High Redshift QSOS Emission Lines in High Redshift QSOS

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3066b&link_type=abstract

HST Proposal ID #3066

Mathematics

Probability

Hst Proposal Id #3066 Quasars &Amp, Agn

Scientific paper

We will use the FOS to measure the strength of the He I lambda 584 line in the UV in a QSO which has a good probability of having light at that wavelength. We will demonstrate the ability of the FOS to detect weak emission lines against a background of weak absorption lines in a faint object with the degraded performance due to the slit losses, decreased resolution, possible increased scattered light and greater than expected particle-induced background. From this line we will determine the relative abundance of Helium in the early universe.

Affiliated with

Also associated with

No associations

Rating

Emission Lines in High Redshift QSOS does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Emission Lines in High Redshift QSOS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emission Lines in High Redshift QSOS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1094247