D. Giles
University of Sydney
4 Papers
58 Citations
D. Giles is an academic researcher from University of Sydney. The author has contributed to research in topics: Atmosphere & Equivalent width. The author has an hindex of 4, co-authored 4 publications.
Chat about Author
Papers
Pluto's atmosphere from the 29 June 2015 ground-based stellar occultation at the time of the New Horizons flyby
Bruno Sicardy,John Talbot,E. Meza,Julio Camargo,Josselin Desmars,D. Gault,D. Herald,S. Kerr,H. Pavlov,Felipe Braga-Ribas,Marcelo Assafin,G. Benedetti-Rossi,A. Dias-Oliveira,A. Ramos-Gomes-Jr.,Roberto Vieira-Martins,Diane Berard,Pierre Kervella,Jean Lecacheux,E. Lellouch,W. Beisker,D. Dunham,Martin Jelínek,Rene Duffard,J. L. Ortiz,A. J. Castro-Tirado,Ronan Cunniffe,Richard Querel,P. A. Yock,Andrew A. Cole,A. B. Giles,K. M. Hill,J. P. Beaulieu,M. Harnisch,R. Jansen,A. Pennell,S. Todd,W. H. Allen,P. B. Graham,B. Loader,G. McKay,J. Milner,S. Parker,M. A. Barry,J. Bradshaw,J. Broughton,L. Davis,Hadrien A. R. Devillepoix,Jack D. Drummond,L. Field,M. Forbes,D. Giles,R. Glassey,R. Groom,D. Hooper,R. Horvat,G. Hudson,R. Idaczyk,D. Jenke,B. Lade,J. Newman,P. Nosworthy,P. Purcell,P. F. Skilton,M. Streamer,M. Unwin,H. Watanabe,G. L. White,Dan M. Watson +67 more
TL;DR: In this paper, the authors present results from a multi-chord Pluto stellar occultation observed on 29 June 2015 from New Zealand and Australia, which occurred only two weeks before the NASA New Horizons flyby of the Pluto system and serves as a useful comparison between ground-based and space results.
40
The structure of Chariklo's rings from stellar occultations
Diane Berard,Bruno Sicardy,Julio Camargo,Josselin Desmars,Felipe Braga-Ribas,J. L. Ortiz,Rene Duffard,Nicolás Morales,E. Meza,Rodrigo Leiva,G. Benedetti-Rossi,Roberto Vieira-Martins,A. R. Gomes-Junior,Marcelo Assafin,F. Colas,Jean-Luc Dauvergne,Pierre Kervella,Jean Lecacheux,L. Maquet,Frédéric Vachier,S. Renner,B. Monard,A. A. Sickafoose,H. Breytenbach,Anja Genade,W. Beisker,K. L. Bath,H.-J. Bode,Michael Backes,Valentin D. Ivanov,Emmanuel Jehin,Michaël Gillon,Jean Manfroid,Joe Pollock,Gonzalo Tancredi,S. Roland,R. Salvo,L. Vanzi,Dave Herald,D. Gault,S. Kerr,H. Pavlov,K. M. Hill,J. Bradshaw,M. A. Barry,A. Cool,B. Lade,Andrew A. Cole,J. Broughton,J. Newman,R. Horvart,D. Maybour,D. Giles,L. Davis,R. A. Paton,B. Loader,A. Pennell,P. D. Jaquiery,Stephane Brillant,Fernando Selman,Christophe Dumas,C. Herrera,G. Carraro,Lorenzo Monaco,Alain Maury,A. Peyrot,J.-P. Teng-Chuen-Yu,Andrea Richichi,Puji Irawati,C. De Witt,P. Schoenau,R. Prager,C. Colazo,R. Melia,J. Spagnotto,A. Blain,S. Alonso,A. Román,Pablo Santos-Sanz,J. L. Rizos,J. L. Maestre,D. Dunham +81 more
TL;DR: In this article, the authors used 12 successful occulations by Chariklo observed between 2014 and 2016 to provide ring profiles (physical width, opacity, edge structure) and constraints on the radii and pole position.
The Structure of Chariklo’s Rings from Stellar Occultations
D. Bérard,Bruno Sicardy,Julio Camargo,Josselin Desmars,Felipe Braga-Ribas,J. L. Ortiz,Rene Duffard,Nicolás Morales,E. Meza,Rodrigo Leiva,G. Benedetti-Rossi,R. Vieira-Martins,A.-R. Gomes Júnior,Marcelo Assafin,François Colas,Jean-Luc Dauvergne,Pierre Kervella,J. Lecacheux,L. Maquet,Frédéric Vachier,S. Renner,B. Monard,A. A. Sickafoose,H. Breytenbach,Anja Genade,W. Beisker,K. L. Bath,H.-J. Bode,Michael Backes,Valentin D. Ivanov,Emmanuel Jehin,Michaël Gillon,Jean Manfroid,Joe Pollock,Gonzalo Tancredi,S. Roland,R. Salvo,L. Vanzi,Dave Herald,D. Gault,S. Kerr,H. Pavlov,K. M. Hill,J. Bradshaw,M. A. Barry,A. Cool,B. Lade,Andrew A. Cole,J. Broughton,J. Newman,R. Horvat,D. Maybour,D. Giles,L. Davis,R. A. Paton,B. Loader,A. Pennell,P. D. Jaquiery,Stephane Brillant,Fernando Selman,Christophe Dumas,C. Herrera,Giovanni Carraro,Lorenzo Monaco,Alain Maury,A. Peyrot,J.-P. Teng-Chuen-Yu,A. Richichi,Puji Irawati,C. De Witt,P. Schoenau,R. Prager,C. Colazo,R. Melia,J. Spagnotto,A. Blain,S. Alonso,A. Román,Pablo Santos-Sanz,J. L. Rizos,J. L. Maestre,D. Dunham +81 more
TL;DR: In this paper, the authors used 12 successful occulations by Chariklo observed between 2014 and 2016 to provide ring profiles (physical width, opacity, edge structure) and constraints on the radii and pole position.
Pluto's atmosphere from the 2015 june 29 ground-based stellar occultation at the time of the new horizons flyby *
Bruno Sicardy,John Talbot,E. Meza,Julio Camargo,Josselin Desmars,D. Gault,D. Herald,S. Kerr,H. Pavlov,Felipe Braga-Ribas,Felipe Braga-Ribas,Marcelo Assafin,G. Benedetti-Rossi,A. Dias-Oliveira,A. R. Gomes-Júnior,R. Vieira-Martins,D. Bérard,Pierre Kervella,Pierre Kervella,J. Lecacheux,E. Lellouch,W. Beisker,D. Dunham,Martin Jelínek,Martin Jelínek,Rene Duffard,J. L. Ortiz,A. J. Castro-Tirado,A. J. Castro-Tirado,Ronan Cunniffe,Richard Querel,P. C. M. Yock,Andrew A. Cole,A. B. Giles,K. M. Hill,J. P. Beaulieu,M. Harnisch,R. Jansen,A. Pennell,S. Todd,W. H. Allen,P. B. Graham,P. B. Graham,B. Loader,G. McKay,J. Milner,S. Parker,M. A. Barry,M. A. Barry,J. Bradshaw,J. Broughton,L. Davis,Hadrien A. R. Devillepoix,Jack D. Drummond,L. Field,M. Forbes,M. Forbes,D. Giles,R. Glassey,R. Groom,D. Hooper,R. Horvat,G. Hudson,R. Idaczyk,D. Jenke,B. Lade,J. Newman,P. Nosworthy,P. Purcell,P. F. Skilton,M. Streamer,M. Unwin,H. Watanabe,G. L. White,Dan M. Watson +74 more
TL;DR: In this article, the authors present results from a multi-chord Pluto stellar occultation observed on 2015 June 29 from New Zealand and Australia, which occurred only two weeks before the NASA New Horizons flyby of the Pluto system and serves as a useful comparison between ground-based and space results.