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Figure 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 1 of 8) A.

Published byElaine Ruby Richardson Modified over 8 years ago

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Presentation on theme: "Figure 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 1 of 8) A."— Presentation transcript:

1 Figure 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 1 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 2 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 3 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 4 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 5 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 6 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 7 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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 6 from HST/WFC3 Near-infrared Spectroscopy of Quenched Galaxies at z ~ 1.5 from the WISP Survey: Stellar Population Properties (Image 8 of 8) A. G. Bedregal et al. 2013 ApJ 778 126 doi:10.1088/0004-637X/778/2/126 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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