Identification of a gravitationally lensed z = 2.515 star-forming galaxy
tometric catalogue of Le Borgne et ai. (1992), is one of .... Since the source lies so
close to a caustic in the source plane, any bright parts of it lying outside this
caustic ... td. Q). 0:: 1. 0.5. 2000. 4500. 5000. 5500. 6000. Observed Wavelength (
A) ... Restframe Wavelength (A). 1200. 1300. 1400. 1500. 1600. 1700. 1. ---.. r:...
'-' 0.Télécharger Identification of a gravitationally lensed z = 2.515 star-forming galaxy pdf
