SPIRE scanmaps of a sample of 200 new Planck sources found all over the sky. The sample includes: 75 Planck Catalogue of Compact Sources high-z SEDs (50 dusty; 25 synchrotron); 100 Planck faint high-z candidates; and 25 SZ clusters. With 14 minutes per AOR to reach the confusion limit on the central virgul10.x10. of a virgul20.x20. field, the identification of the sources will be straightforward.
Publication
Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE | Planck Collaboration Aghanim et al. | Astronomy & Astrophysics Volume 582 id.A30 29 pp. | 582 | 10.1051\\/0004-6361\\/201424790 | 2015A&A...582A..30P | http://adsabs.harvard.edu/abs/2015A%26A...582A..30P
Instrument
SPIRE_SpirePhoto_large
Temporal Coverage
2012-10-29T13:28:37Z/2013-04-16T23:54:07Z
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, pilbratt et al., 2013, 'The Herschel & Planck All-Sky Source Snapshot Legacy Survey', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-w1r14gw
