VizieR Online Data Catalog: Total/polarized extinction/emission PostPlanck Era (Hensley+, 2021)

Extinction. From 0.55 to 2.2μm, we employ the extinction curve of Schlafly+, 2016ApJ...821...78S assuming A_H/A_K=1.55. From 2.2 to 37μm, we adopt the MIR extinction curve derived by Hensley & Draine, 2020, J/ApJ/895/38 on the sight line toward Cyg OB2-12.

Polarized extinction. Between 0.12 and 4μm, we join a Serkowski law with parameters K=0.87 and λ_max=0.55μm smoothly to a power law with index β=1.6 in the IR.

Emission. In the MIR, we adopt the AKARI and Spitzer spectrum of a sample of PAH-bright galaxies (Lai+, 2020ApJ...905...55L) between 3 and 12μm and the Spitzer IRS observations of the translucent cloud DCld 300.2-16.9 between 6 and 38μm.In the FIR, we adopt the HI-correlated dust emission measured in the DIRBE and Planck bands with ν>=353GHz, and the 353GHz-correlated emission measured in the lower frequency Planck and WMAP bands by Planck Collaboration Int. XXII (2015A&A...576A.107P).

Polarized emission. We adopt the frequency dependence of the polarized infrared emission determined by Planck Collaboration XI (2020A&A...641A..11P) scaled to match the relation between polarized extinction and emission derived by Planck Collaboration XII (2020A&A...641A..12P).

(4 data files).