Integral-field spectroscopy and HST imaging of ULIRGs at low and high redshift: IRAS 16007+3743

Details Integral-field spectroscopy and HST imaging of ULIRGs at low and high redshift: IRAS 16007+3743 Integral-field spectroscopy and HST imaging of ULIRGs at low and high redshift: IRAS 16007+3743

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329p..19g&link_type=abstract

Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results of the Ultraluminous Infrared Galaxy (ULIRG) IRAS 16007+3743 (z=0.18), as part of an ongoing program aimed at studying the internal physical structure and kinematics of a representative sample of ULIRGs (see Colina et al., 2004, and references therein). The program is based on integral-field spectroscopy data from the INTEGRAL system (WHT), and HST imaging. With these data we characterize this system and perform preliminary high-redshift simulations of future instruments such as JWST NIRSpec, MIRI and NIRCam, which will be useful to establish the connection between the local ULIRGs and high-z galaxies (LBGs, SMGs).

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