2019MNRAS.487.5814V


Query : 2019MNRAS.487.5814V

2019MNRAS.487.5814V - Mon. Not. R. Astron. Soc., 487, 5814-5823 (2019/August-3)

Statistical properties of polarized CMB foreground maps.

VON HAUSEGGER S., GAMMELGAARD RAVNEBJERG A. and LIU H.

Abstract (from CDS):

Foreground removal techniques for CMB analyses make specific assumptions about the properties of foregrounds in temperature and in polarization. By investigating the statistics of foreground components more understanding about the degree to which these assumptions are valid can be obtained. In this work we investigate E- and B-mode maps of the two strongest polarized foregrounds, synchrotron and thermal dust emission, with regards to their similarity with Gaussian processes, their spectral variations, and cross-correlations. We perform tests in patches of ∼3.7° size collectively covering the full sky and find most of them to conform to their Gaussian expectation according to the statistics in use. Correlations exhibit distinct differences in E- and B-mode signals, which point towards necessities in foreground removal methods. We discuss potential consequences and possible further directions.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): methods: data analysis - methods: statistical - cosmic background radiation - cosmology: observations

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME North Polar Spur ISM 12 00 +00.0           ~ 405 1

Query : 2019MNRAS.487.5814V

Basic data :
NAME North Polar Spur -- Interstellar Medium Object
Other object types:
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ISM ()
ICRS coord. (ep=J2000) :
12 00 00.0 +00 00 00 [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
11 57 26.2 +00 16 42 [ ]
Gal coord. (ep=J2000) :
276.3373 +60.1886 [ ]
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Identifiers (2) :
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NAME NPS NAME North Polar Spur

References (405 between 1850 and 2026) (Total 405)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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