Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 3, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2016/03/023
Keywords
CMBR experiments; supernova remnants
Funding
- National Natural Science Foundation of China [11033003]
- National Natural Science Foundation for Young Scientists of China [11203024]
- Youth Innovation Promotion Association, CAS
- DoE [DE-AC02-76SF00515]
- KIPAC Kavli Fellowship
- Science and Technology Facilities Council [ST/L000474/1, PP/C506205/1, ST/J000507/1] Funding Source: researchfish
- Villum Fonden [00010056] Funding Source: researchfish
- STFC [ST/J000507/1, PP/C506205/1, ST/L000474/1] Funding Source: UKRI
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Cosmology has made enormous progress through studies of the cosmic microwave background, however the subtle signals being now sought such as B-mode polarisation due to primordial gravitational waves are increasingly hard to disentangle from residual Galactic foregrounds in the derived CMB maps. We revisit our finding that on large angular scales there are traces of the nearby old supernova remnant Loop I in the WMAP 9-year map of the CMB and confirm this with the new SMICA map from the Planck satellite.
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