Sources of uncertainty in the relative scaling of spectroscopic data

Details Sources of uncertainty in the relative scaling of spectroscopic data Sources of uncertainty in the relative scaling of spectroscopic data

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..103..121b&link_type=abstract

Astronomy and Astrophysics Suppl. 103, 121-128 (1994)

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

We discuss in this paper the various sources of uncertainty which arise in the relative scaling of spectroscopic data sets obtained on active galactic nuclei. The case is illustrated for NGC 3227, one of the targets monitored during the LAG campaign, and the errors derived have been attached to the final results discussed by Salamanca et al. (1993). We examine the effects of slit miscentering, of differences in the atmospheric seeing and finally of the line deblending procedure.

Affiliated with

Also associated with

No associations

Rating

Sources of uncertainty in the relative scaling of spectroscopic data 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 Sources of uncertainty in the relative scaling of spectroscopic data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sources of uncertainty in the relative scaling of spectroscopic data will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-863191