GPI Spectra of HR 8799 c, d, and e from 1.5 to 2.4 μm with KLIP Forward Modeling
- Author(s):
- Greenbaum, A.Z.; Pueyo, L.; Ruffio, J.B.; Wang, J.J.; De Rosa, R.J.; Aguilar, J.; Rameau, J.; Barman, T.; Marois, C.; Marley, M.S.; Konopacky, Q.; Rajan, A.; Macintosh, B.; Ansdell, M.; Arriaga, P.; Bailey, V.P.; Bulger, J.; Burrows, A.; Chilcote, J.; Cotten, T.; Doyon, R.; Duchêne, G.; Fitzgerald, M.P.; Follette, K.B.; Gerard, B.; Goodsell, S.J.; Graham, J.R.; Hibon, P.; Hung, L.W.; Ingraham, P.; Kalas, P.; Larkin, J.E.; Maire, J.; Marchis, F.; Metchev, S.; Millar-Blanchaer, M.A.; Nielsen, E.L.; Norton, A.; Oppenheimer, R.; Palmer, D.; Patience, J.; Perrin, M.D.; Poyneer, L.; Rantakyrö, F.T.; Savransky, D.; Schneider, A.C.; Sivaramakrishnan, A.; Song, I.; Soummer, R.; Thomas, S.; Wallace, J.K.; Ward-Duong, K.; Wiktorowicz, S.; Wolff, S.
- Published
- 2018
- Publication type
- Article / Letter to editor
- Date issued
- 2018
- Language
- English
- Is part of
- The Astronomical Journal (2018), Vol. 155, no. 6, p. 226
- hdl
- 1887/69650
- doi
- 10.3847/1538-3881/aabcb8
- URL
- https://ui.adsabs.harvard.edu/#abs/2018AJ....155..226G
