1. Multi-wavelength galaxy surveys at the North Ecliptic Pole: from Herschel & AKARI to Euclid & SPICA Stephen Serjeant JCMT UK meeting, September 2014

2. AKARI: Japanese/Korean mission 2006-2011

3. AKARI Deep area covered by SCUBA2 (0.5 deg 2 ) Wide area covered by Herschel (9 deg 2 )

6. Murata et al. 2014 A&A PAH deficit above the “main sequence”

7. V. Buat 8  m rest- frame selected sample

8. Euclid (launch 2020) Source: Euclid 2009 yellow book Wide survey: 15,000 deg 2 (above) Deep survey: ~2 mag deeper, ~40 deg 2

9. NEP & East Asian surveys Ideal location for probing solid-state phases of ISM and e.g. connection to “main sequence” thanks to AKARI SCUBA-2 survey over 0.5 deg 2 to 8mJy in CLS Future deep field for SPICA, Euclid etc