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- W3099604751 abstract "We present near-infrared observations of the ultraluminous high-redshift (z = 2.286) IRAS source FSC 10214+4724 obtained in 04 seeing at the W. M. Keck telescope. These observations show that FSC 10214+4724 consists of a highly symmetric circular arc centered on a second weaker source. The arc has an angular extent of about 140° and is probably unresolved in the transverse direction. This morphology constitutes compelling prima facie evidence for a gravitationally lensed system. Our images also contain evidence for the faint counterimage predicted by the lens hypothesis. The morphology of FSC 10214+4724 can be explained in terms of a gravitationally lensed background source if the object at the center of curvature of the arc is an L* galaxy at z ≈ 0.7. If FSC 10214+4724 is lensed, then there is significant magnification and its luminosity has been overestimated by a large factor. Our results suggest that FSC 10214+4724 is not a uniquely luminous object but ranks among the most powerful quasars and ultraluminous IRAS galaxies." @default.
- W3099604751 created "2020-11-23" @default.
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- W3099604751 date "1995-08-10" @default.
- W3099604751 modified "2023-10-14" @default.
- W3099604751 title "High-Resolution Infrared Imaging of FSC 10214+4724: Evidence for Gravitational Lensing" @default.
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- W3099604751 doi "https://doi.org/10.1086/309629" @default.
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