期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 728, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/728/1/L18
关键词
galaxies: clusters: general; gravitational lensing: strong; quasars: individual (SDSS 102913.94+262317.9)
资金
- Alfred P. Sloan Research Fellowship
- NSF [AST-0708082, AST-1009756]
- US Department of Energy by Lawrence Livermore National Laboratory [W-7405-ENG-48]
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1009756] Funding Source: National Science Foundation
Using a high-resolution radio image, we successfully resolve the two-fold image components B and C of the quasar lens system SDSS J1029+2623. The flux anomalies associated with these two components in the optical regime persist, albeit less strongly, in our radio observations suggesting that the cluster must be modeled by something more than a single central potential. We argue that placing substructure close to one of the components can account for a flux anomaly with negligible changes in the component positions. Our best-fit model has a substructure mass of similar to 10(9) M-circle dot up to the mass-sheet degeneracy, located roughly 0 ''.1 west and 0 ''.1 north of component B. We demonstrate that a positional offset between the centers of the source components can explain the differences between the optical and radio flux ratios.
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