Gravitationally Lensed Galaxy Number Counts in the Infrared II: Concrete Examples

Details Gravitationally Lensed Galaxy Number Counts in the Infrared II: Concrete Examples Gravitationally Lensed Galaxy Number Counts in the Infrared II: Concrete Examples

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000isass..14..171y&link_type=abstract

The Institute of Space and Astronautical Science Report SP No. 14, p. 171-177.

Astronomy and Astrophysics

Astronomy

Galaxy Number Count, Galaxy Evolution, Cluster Of Galaxies, Gravitational Lens, Infrared Galaxies

Scientific paper

following the concept presented by Takeuchi, Yoshikawa, & Yonehara (2000), we show some concrete examples of number count of lensed galaxies in the infrared. Adopting a simple lens model of cluster of galaxies, we are able to estimate the expected number counts of galaxies. The result tells us that the expected number counts of galaxies around a single cluster are not so large, but in principle, we can discriminate global history of galaxy evolution efficiently at longer waveband, i.e. FIR and/or sub-mm.

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