Persistent URL of this record https://hdl.handle.net/1887/69650
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- 1804.07774
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GPI Spectra of HR 8799 c, d, and e from 1.5 to 2.4 μm with KLIP Forward Modeling
- All authors
- 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.
- Date
- 2018
- Journal
- The Astronomical Journal
- Volume
- 155
- Issue
- 6
- Pages
- 226