Planck's dusty GEMS III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5

Planck's dusty GEMS III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5

We study the properties of the foreground galaxy of the Ruby, the brightest gravitationally lensed high-redshift galaxy on the sub-millimeter sky as probed by the Planck satellite, and part of our sample of Planck's dusty GEMS. The Ruby consists of an Einstein ring of 1.4" diameter at z =...

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Bibliographic Details
Main Authors: Canameras, R., Nesvadba, N. P. H., Kneissl, R., Limousin, M., Gavazzi, R., Scott, D., Dole, H., Frye, B., Koenig, S., Le Floc'h, E., Oteo, I.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: EDP SCIENCES S A 2017
Subjects:
galaxies: high-redshift
galaxies: evolution
galaxies: star formation
galaxies: stellar content
infrared: galaxies
submillimeter: galaxies
Online Access:http://hdl.handle.net/10150/624365
http://arizona.openrepository.com/arizona/handle/10150/624365

Internet

http://hdl.handle.net/10150/624365
http://arizona.openrepository.com/arizona/handle/10150/624365

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