Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S295(8), p. 53-54, 2012

DOI: 10.1017/s1743921313004249

American Astronomical Society, Astrophysical Journal, 2(768), p. 164, 2013

DOI: 10.1088/0004-637x/768/2/164

Links

Tools

Export citation

Search in Google Scholar

High resolution near-infrared imaging of submillimeter galaxies

Journal article published in 2012 by Paula Aguirre, Andrew J. Baker ORCID, Felipe Menanteau, Dieter Lutz ORCID, Linda J. Tacconi
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Upload
Green circle
Postprint: archiving allowed
Upload
Red circle
Published version: archiving forbidden
Policy details
Data provided by SHERPA/RoMEO

Abstract

AbstractWe have obtained high-resolution F110W (~ J) and F160W (~ H) band observations of ten submillimeter galaxies (SMGs) with the Hubble Space Telescope's NICMOS camera, in order to resolve their rest-frame optical morphologies, determine the existence of multiple-component, merger-like configurations, and estimate their stellar masses. The selected targets have redshifts in the range 2.2≤ z ≤ 2.81 confirmed with millimeter or mid-IR spectroscopy, guaranteeing that the two bands sample the galaxies' rest-frame optical light with the Balmer break falling between them.

Beta version