Dust at High Redshift

Details Dust at High Redshift Dust at High Redshift

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...11h&link_type=abstract

Spitzer Proposal ID #11

Physics

Scientific paper

The goal is to probe the properties of dust at high redshifts by obtaining the spectra of sources where the infrared emission is believed to be thermal dust emission. The presence/absence of PAH/Silicate emission/absorption in these systems will address the evolution of the dust content in systems at significant lookback times. The targets chosen are all z>0.9 in which a strong dust continuum has been detected.

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