Figure 1 from Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet

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Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet

Authors: Abhijith Rajan, Julien Rameau, Robert J. De Rosa, Mark S. Marley, James R. Graham, Bruce Macintosh, Christian Marois, Caroline Morley, Jennifer Patience, Laurent Pueyo, Didier Saumon, Kimberly Ward-Duong, S. Mark Ammons, Pauline Arriaga, Vanessa P. Bailey, Travis Barman, Joanna Bulger, Adam S. Burrows, Jeffrey Chilcote, Tara Cotten, Ian Czekala, Rene Doyon, Gaspard Duchêne, Thomas M. Esposito, Michael P. Fitzgerald, Katherine B. Follette, Jonathan J. Fortney, Stephen J. Goodsell, Alexandra Z. Greenbaum, Pascale Hibon, Li-Wei Hung, Patrick Ingraham, Mara Johnson-Groh, Paul Kalas, Quinn Konopacky, David Lafrenière, James E. Larkin, Jérôme Maire, Franck Marchis, Stanimir Metchev, Maxwell A. Millar-Blanchaer, Katie M. Morzinski, Eric L. Nielsen, Rebecca Oppenheimer, David Palmer, Rahul I. Patel, Marshall Perrin, Lisa Poyneer, Fredrik T. Rantakyrö, Jean-Baptiste Ruffio, Dmitry Savransky, Adam C. Schneider, Anand Sivaramakrishnan, Inseok Song, Rémi Soummer, Sandrine Thomas, Gautam Vasisht, J. Kent Wallace, Jason J. Wang, Sloane Wiktorowicz, and Schuyler Wolff

2017 The Astronomical Journal 154 10.

Provider: AAS Journals

Caption: Figure 1.

Final PSF-subtracted images of 51 Eri b. Top: LOCI-reduced GPIES images at the K1 (2016 January 28, left) and K2 bands (2015 December 18, right). Bottom: pyKLIP-reduced NIRC2 images, smoothed with a box of width 2 pixels, at L_P (2015 October 27, left), and a combined image of all four M_S data sets (right). The images are scaled linearly, but are different in each panel in order to saturate the core of the planet PSF.

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