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2018AJ....155..226G - Astron. J., 155, 226-226 (2018/June-0)
GPI spectra of HR 8799 c, d, and e from 1.5 to 2.4 µm with KLIP forward modeling.
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.S., CHILCOTE J., COTTEN T., DOYON R., DUCHENE 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., RANTAKYRO F.T., SAVRANSKY D., SCHNEIDER A.C., SIVARAMAKRISHNAN A., SONG I., SOUMMER R., THOMAS S., WALLACE J.K., WARD-DUONG K., WIKTOROWICZ S. and WOLFF S.
Abstract (from CDS):
Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.
Journal keyword(s): planets and satellites: gaseous planets - stars: individual: HR 8799
VizieR on-line data: <Available at CDS (J/AJ/155/226): table3.dat>
Simbad objects: 10
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