HerMES: Current Cosmic Infrared Background Estimates Can be Explained by Known Galaxies and their Faint Companions at z < 4 (Viero et al. 2015; arXiv:1505.06242)

1. Herschel/SPIRE maps with 4 arcsec pixels
   

2. Cumulative measured CIB vs. Effective Image Resolution (Figure 1: LaTex)
   

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HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift (Viero et al. 2013b; arXiv:1304.0446)

1. 
   

2. [L-M*-z] Generation Code (Figure 8: IDL)
   

3. Total Stacked Intensities (Table 3: ascii)
   

4. Stacked Flux Densities of Star-Forming Galaxies (Table 4: IDL)
   

5. Stacked Flux Densities of Quiescent Galaxies (Table 5: IDL)
   

6. Stacked Intensities in Redshift Bins (Table 6: IDL)
   

7. Stacked Intensities in Stellar Mass Bins for Star-Forming Galaxies (Table 7: IDL)
   

8. Stacked Intensities in Stellar Mass Bins for Quiescent Galaxies (Table 8: IDL)
   

9. Redshift Distribution of Resolved CIB Emission (Figure 12: IDL)
   

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HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies (Viero et al. 2013a; arXiv:1208.5049)

1. Auto and Cross-Frequency Power Spectra (Table 10)
   

2. Halo Model
   

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Correlations in the (Sub)millimeter Background from ACT×BLAST

(Hajian, Viero et al. 2012; arXiv:1101.1517)

1. BLAST×BLAST and ACT×BLAST Power Spectra