Published October 1, 2012 | Version v1
Journal article

A BAYESIAN MONTE CARLO ANALYSIS OF THE M-σ RELATION

  • 1. Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 (United States)

Description

We present an analysis of selection biases in the Mbh-σ relation using Monte Carlo simulations including the sphere of influence resolution selection bias and a selection bias in the velocity dispersion distribution. We find that the sphere of influence selection bias has a significant effect on the measured slope of the Mbh-σ relation, modeled as βintrinsic = –4.69 + 2.22βmeasured, where the measured slope is shallower than the model slope in the parameter range of β > 4, with larger corrections for steeper model slopes. Therefore, when the sphere of influence is used as a criterion to exclude unreliable measurements, it also introduces a selection bias that needs to be modeled to restore the intrinsic slope of the relation. We find that the selection effect due to the velocity dispersion distribution of the sample, which might not follow the overall distribution of the population, is not important for slopes of β ∼ 4-6 of a logarithmically linear Mbh-σ relation, which could impact some studies that measure low (e.g., β < 4) slopes. Combining the selection biases in velocity dispersions and the sphere of influence cut, we find that the uncertainty of the slope is larger than the value without modeling these effects and estimate an intrinsic slope of β = 5.28+0.84–0.55.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/757/2/172

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
757
Journal Issue
2
Journal Page Range
[9 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
44050425
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ASTRONOMY; ASTROPHYSICS; BLACK HOLES; COMPUTERIZED SIMULATION; CORRECTIONS; GALAXIES; MONTE CARLO METHOD; RESOLUTION; VELOCITY
Descriptors DEC
CALCULATION METHODS; PHYSICS; SIMULATION