Figure 2 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Transmission Spectrum of the Potentially Rocky Planet L 98-59 c

Authors: Thomas Barclay, Kyle B. Sheppard, Natasha Latouf, Avi M. Mandell, Elisa V. Quintana, Emily A. Gilbert, Giuliano Liuzzi, Geronimo L. Villanueva, Giada Arney, Jonathan Brande, Knicole D. Colón, Giovanni Covone, Ian J. M. Crossfield, Mario Damiano, Shawn D. Domagal-Goldman, Thomas J. Fauchez, Stefano Fiscale, Francesco Gallo, Christina L. Hedges, Renyu Hu, Edwin S. Kite, Daniel Koll, Ravi K. Kopparapu, Veselin B. Kostov, Laura Kreidberg, Eric D. Lopez, James Mang, Caroline V. Morley, Fergal Mullally, Susan E. Mullally, Daria Pidhorodetska, Joshua E. Schlieder, Laura D. Vega, Allison Youngblood, Sebastian Zieba

Thomas Barclay et al 2025 The Astronomical Journal 169 .

Provider: AAS Journals

Caption: Figure 2.

Visualization of white-light light-curve fit for the highest-weighted systematic model for L 98-59 c, which demonstrates a good model fit to the observed data. Panel (a) shows the band-integrated light curve. Panel (b) shows the detrended light curve as well as the best-fitting transit model. The instrumental effects and transit model parameters were fit for simultaneously. Panel (c) shows the residuals between the data and the best-fitting model.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions