We propose Herschel/SPIRE photometric observations of dust continuum emission in a sample of 19 weak line quasars (WLQs) at 2
Publication
Instrument
SPIRE_SpirePhoto_small
Temporal Coverage
2012-02-29T18:29:19Z/2013-01-20T06:03:47Z
Version
SPG v14.1.0
Mission Description
Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
European Space Agency, wang et al., 2013, 'Dust Emission and Star Forming Activity in the High Redshift Weak Line Quasars', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-3061dl0