Selection Bias in Observing the Cosmological Evolution of the Mbh-sigma and Mbh-L Relationships

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

28 pages, 6 figures, submitted to the Astrophysical Journal

Scientific paper

10.1086/522083

Programs to observe evolution in the Mbh-sigma or Mbh-L relations typically compare black-hole masses, Mbh, in high-redshift galaxies selected by nuclear activity to Mbh in local galaxies selected by luminosity L, or stellar velocity dispersion sigma. Because AGN luminosity is likely to depend on Mbh, selection effects are different for high-redshift and local samples, potentially producing a false signal of evolution. This bias arises because cosmic scatter in the Mbh-sigma and Mbh-L relations means that the mean log(L) or log(sigma) among galaxies that host a black hole of given Mbh, may be substantially different than the log(L) or log(sigma) obtained from inverting the Mbh-L or Mbh-sigma relations for the same nominal Mbh. The bias is particularly strong at high Mbh, where the luminosity and dispersion functions of galaxies are falling rapidly. The most massive black holes occur more often as rare outliers in galaxies of modest mass than in the even rarer high-mass galaxies, which would otherwise be the sole location of such black holes in the absence of cosmic scatter. Because of this bias, Mbh will typically appear to be too large in the distant sample for a given L or sigma. For the largest black holes and the largest plausible cosmic scatter, the bias can reach a factor of 3 in Mbh for the Mbh-sigma relation and a factor of 9 for the Mbh-L relation. Unfortunately, the actual cosmic scatter is not known well enough to correct for the bias. Measuring evolution of the Mbh and galaxy property relations requires object selection to be precisely defined and exactly the same at all redshifts.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Selection Bias in Observing the Cosmological Evolution of the Mbh-sigma and Mbh-L Relationships 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 Selection Bias in Observing the Cosmological Evolution of the Mbh-sigma and Mbh-L Relationships, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Selection Bias in Observing the Cosmological Evolution of the Mbh-sigma and Mbh-L Relationships will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-498801

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.