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Figure 1 from Characterizing the Cool KOIs. VI

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Presentation on theme: "Figure 1 from Characterizing the Cool KOIs. VI"— Presentation transcript:

1 Figure 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 1 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 2 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 3 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 4 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 5 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 6 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 7 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 8 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 9 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 10 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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 1 from Characterizing the Cool KOIs. VI
Figure 1 from Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-candidate Hosts (Image 11 of 11) Philip S. Muirhead et al ApJS doi: / /213/1/5 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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