![](images/OutreachMaterial/SpitzerHerschelBandpasses.jpg)
Outreach Material
Feel free to use any of the following outreach materials for any non-commercial application. Please, do cite the KINGFISH LEGACY (or the corresponding paper if mentioned) when using them.
For commercial use, please contact us.
Images
Talks
Visuals
Press Releases
Images
![](images/OutreachMaterial/SpitzerHerschelBandpasses.jpg)
The Herschel filter bandpasses are shown at the bottom of the figure. (Kennicutt et al. 2011)
![](images/OutreachMaterial/MIPSversusPACS.jpg)
Note the improvment in terms of spatial resolution between the two instruments. (Kennicutt et al. 2011)
![](images/OutreachMaterial/NGC0628_Multiwavelength.jpg)
Top: Spitzer images at 3.6 μm, 8.0 μm and 24 μm. The emissionis dominated by stars, small PAH grains, and small dust grains heated by intense radiatino fields, respectively.
Middle: Herschel PACS images at 70 μm, 100 μm, and 160 μm. Note the progressive increase in contributions from diffuse dust emission with increasing wavelength.
Bottom: Herschel SPIRE images at 250 μm, 350 μm, and 500 μm. These bands trace increasingly cooler components of the main thermal dust emission.