Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization

Home

All issues

Volume 576 (April 2015)

A&A, 576 (2015) A107

Full HTML

Free Access

Table 5

Polarized dust spectral indices derived using multiple subsets and templates of the Planck data.

Templates	Data sets

..............	Full	1.592
..............	HR1	1.595
DS1 and DS2 .....	HR2	1.595
..............	YR1	1.619
..............	YR2	1.592

..............	Full	1.602
..............	HR1	1.603
YR1 and YR2 .....	HR2	1.606
..............	DS1	1.564
..............	DS2	1.627

..............	Full	1.613
..............	DS1	1.579
HR1 and HR2 .....	DS2	1.639
..............	YR1	1.639
..............	YR2	1.614

..............	Full	1.578
..............	DS1	1.560
S1+S3 and S2+S4 .....	DS2	1.590
..............	HR1	1.581
..............	HR2	1.588

Notes. The full mission Planck polarization data along with the DS1 and DS2 templates (first entry in the Table below) is used in Sect. 8.1 to produce Fig. 9. The scatter of the 20 measurements is consistent with the 1σ statistical uncertainty on the mean value of .

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.