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Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans.

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Presentation on theme: "Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans."— Presentation transcript:

1 Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 1 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 2 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 3 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 4 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 5 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 6 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 7 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 8 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 9 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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.

10 Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 10 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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.

11 Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 11 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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.

12 Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 12 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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.

13 Figure 2 from Lifting the Dusty Veil with Near- and Mid-infrared Photometry. III. Two-dimensional Extinction Maps of the Galactic Midplane Using the Rayleigh–Jeans Color Excess Method (Image 13 of 13) David L. Nidever et al ApJS doi: / /201/2/35 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal Supplement Series. 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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