Andromeda vs Milky Way dust emissions

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SUMMARY

The discussion centers on the implications of the Planck XXV release, which mapped dust emissions in Andromeda, for the BICEP 2 findings on primordial gravity waves. Participants express disappointment that the Planck XXV paper did not address its relevance to BICEP 2's dust modeling, particularly regarding foreground B-modes. The consensus suggests that using Andromeda's data may not resolve the issues raised about BICEP 2's methodology, and further verification or reanalysis is necessary to clarify the situation. The full Planck results are anticipated in October, which may provide additional insights.

PREREQUISITES
  • Understanding of primordial gravity waves and their significance in cosmology.
  • Familiarity with BICEP 2's methodology for detecting gravitational waves.
  • Knowledge of Planck satellite data and its role in cosmic microwave background studies.
  • Basic grasp of foreground B-modes and their impact on gravitational wave detection.
NEXT STEPS
  • Research the full Planck results scheduled for release in October.
  • Examine the paper "http://arxiv.org/abs/1407.5452" for detailed insights into BICEP 2's findings.
  • Investigate the implications of E-mode coupling in gravitational wave studies.
  • Explore alternative data sets for foreground tensor perturbations in cosmological research.
USEFUL FOR

Astronomers, cosmologists, and researchers involved in gravitational wave detection and analysis, particularly those interested in the interplay between dust emissions and cosmic background radiation.

Chronos
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As many are aware, the announced detection of primordial gravity waves by BICEP 2 was heavily criticized based on dust emission modeling. Today, Planck XXV was released which mapped out the dust emissions of Andromeda. Assuming Andromeda is representative of the Milky Way in most relevant ways, the obvious question is does Planck XXV affirm, cast further doubt upon, or is irrelevant to BICEP 2 dust modeling? I was perhaps naively disappointed this was never mentioned in the paper. The paper of interest is http://arxiv.org/abs/1407.5452,
 
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Chronos said:
As many are aware, the announced detection of primordial gravity waves by BICEP 2 was heavily criticized based on dust emission modeling. Today, Planck XXV was released which mapped out the dust emissions of Andromeda. Assuming Andromeda is representative of the Milky Way in most relevant ways, the obvious question is does Planck XXV affirm, cast further doubt upon, or is irrelevant to BICEP 2 dust modeling? I was perhaps naively disappointed this was never mentioned in the paper. The paper of interest is http://arxiv.org/abs/1407.5452,

Seems like the paper would be mostly irrelevant; considering the controversy was about the BICEP teams handing of foreground B-modes and the data (or lack thereof) they used. Using Andromeda's data set to calculate foreground tensor perturbations might not be any better than the incomplete set they used I would assume. Full Planck results come out in October right? Only a second verification by another group, or an in-depth reanalysis with a full data set would squash this discussion one way or another.

What if it all turns out to be an E-mode coupling issue. :-p

Anyway, GR still confuses the hell out of me, mostly.
 

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