SIMBAD references

2013ApJ...769...52W - Astrophys. J., 769, 52 (2013/May-3)

A new approach to identifying the most powerful gravitational lensing telescopes.

WONG K.C., ZABLUDOFF A.I., AMMONS S.M., KEETON C.R., HOGG D.W. and GONZALEZ A.H.

Abstract (from CDS):

The best gravitational lenses for detecting distant galaxies are those with the largest mass concentrations and the most advantageous configurations of that mass along the line of sight. Our new method for finding such gravitational telescopes uses optical data to identify projected concentrations of luminous red galaxies (LRGs). LRGs are biased tracers of the underlying mass distribution, so lines of sight with the highest total luminosity in LRGs are likely to contain the largest total mass. We apply this selection technique to the Sloan Digital Sky Survey and identify the 200 fields with the highest total LRG luminosities projected within a 3.'5 radius over the redshift range 0.1 ≤ z ≤ 0.7. The redshift and angular distributions of LRGs in these fields trace the concentrations of non-LRG galaxies. These fields are diverse; 22.5% contain one known galaxy cluster and 56.0% contain multiple known clusters previously identified in the literature. Thus, our results confirm that these LRGs trace massive structures and that our selection technique identifies fields with large total masses. These fields contain two to three times higher total LRG luminosities than most known strong-lensing clusters and will be among the best gravitational lensing fields for the purpose of detecting the highest redshift galaxies.

Abstract Copyright:

Journal keyword(s): galaxies: clusters: general - gravitational lensing: strong

VizieR on-line data: <Available at CDS (J/ApJ/769/52): table1.dat table2.dat table3.dat>

Status at CDS:  

Simbad objects: 278

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2013ApJ...769...52W and select 'bookmark this link' or equivalent in the popup menu


2020.03.31-01:55:58

© Université de Strasbourg/CNRS

    • Contact