The FIRST project: a single-mode fiber-based very high-dynamic range diffraction-limited imaging instrument at visible to near-infrared wavelengths
暂无分享,去创建一个
Pierre Kervella | Stephen T. Ridgway | Takayuki Kotani | Daniel Rouan | Pierre Fedou | Olivier Chesneau | Guy Perrin | Jean-Philippe Berger | Sylvestre Lacour | Olivier Lai | Alfred Vidal-Madjar | Eric Thiébaut | Julien Woillez | Pascal Bordé | Alain Lecavelier | G. Perrin | É. Thiébaut | S. Ridgway | D. Rouan | P. Bordé | S. Lacour | O. Chesneau | J. Woillez | J. Berger | T. Kotani | O. Lai | P. Kervella | A. Vidal-Madjar | P. Fédou | A. Lecavelier
[1] G. P. Weigelt,et al. Modified astronomical speckle interferometry “speckle masking” , 1977 .
[2] G. Perrin,et al. High dynamic range imaging by pupil single‐mode filtering and remapping , 2006 .
[3] P. Tuthill,et al. Michelson Interferometry with the Keck I Telescope , 2000 .
[4] E. K. Baines,et al. First Results from the CHARA Array. I. An Interferometric and Spectroscopic Study of the Fast Rotator α Leonis (Regulus) , 2005 .
[5] Craig D. Mackay,et al. The point spread function in Lucky Imaging and variations in seeing on short timescales , 2008 .
[6] C. A. Haniff,et al. The first images from optical aperture synthesis , 1987, Nature.
[7] Rafael Millan-Gabet,et al. Michigan Infrared Combiner (MIRC): commissioning results at the CHARA Array , 2006, SPIE Astronomical Telescopes + Instrumentation.
[8] G. Perrin,et al. High dynamic range imaging with a single-mode pupil remapping system: a self-calibration algorithm for redundant interferometric arrays , 2006 .
[9] O. Guyon. LIMITS OF ADAPTIVE OPTICS FOR HIGH-CONTRAST IMAGING , 2005, astro-ph/0505086.
[10] Wesley A. Traub,et al. FLUOR fibered instrument at the IOTA interferometer , 1998, Astronomical Telescopes and Instrumentation.
[11] Ray Bell,et al. Subelectron read noise at MHz pixel rates , 2001, IS&T/SPIE Electronic Imaging.
[12] M. Mayor,et al. A Jupiter-mass companion to a solar-type star , 1995, Nature.
[13] S. Seager,et al. PHOTOMETRIC LIGHT CURVES AND POLARIZATION OF CLOSE-IN EXTRASOLAR GIANT PLANETS , 2000 .
[14] A. Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images , 1970 .