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Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image.

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Presentation on theme: "Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image."— Presentation transcript:

1 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 1 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

2 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 2 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

3 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 3 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

4 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 4 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

5 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 5 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

6 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 6 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

7 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 7 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

8 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 8 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

9 Figure 15 from Spectral Energy Distributions of QSOs at z > 5: Common Active Galactic Nucleus-heated Dust and Occasionally Strong Star-formation (Image 9 of 9) C. Leipski et al. 2014 ApJ 785 154 doi:10.1088/0004-637X/785/2/154 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

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