The Four‐Quadrant Phase Mask Coronagraph. IV. First Light at the Very Large Telescope
暂无分享,去创建一个
A. Boccaletti | P. Baudoz | P. Riaud | D. Rouan | A. Lagrange | F. Lacombe | J. Baudrand | D. Gratadour | Damien Gratadour | Francois Lacombe | Anne-Marie Lagrange | F. Lacombe | A. Lagrange
[1] Bradford A. Smith,et al. A Circumstellar Disk Around β Pictoris , 1984, Science.
[2] J. Matsuoka,et al. Temperature dependence of refractive index of SiO2 glass , 1991 .
[3] F. Roddier,et al. STELLAR CORONOGRAPH WITH PHASE MASK , 1997 .
[4] Robert Pina,et al. A dust disk surrounding the young A star HR4796A , 1998 .
[5] Pierre Baudoz,et al. Achromatic interfero coronagraphy - II. Effective performance on the sky , 2000 .
[6] A. Labeyrie,et al. The Four-Quadrant Phase-Mask Coronagraph. I. Principle , 2000 .
[7] Pierre Riaud,et al. The Four‐Quadrant Phase‐Mask Coronagraph. II. Simulations , 2001 .
[8] P. Nisenson,et al. Detection of Earth-like Planets Using Apodized Telescopes , 2001, astro-ph/0101241.
[9] Hst/nicmos2 coronagraphic observations of the circumstellar environment of three old pms stars: hd 100546, sao 206462 and mwc 480 , 2000, astro-ph/0009496.
[10] W. Traub,et al. A Coronagraph with a Band-limited Mask for Finding Terrestrial Planets , 2002, astro-ph/0203455.
[11] Pierre Riaud,et al. Speckle Symmetry with High-Contrast Coronagraphs , 2002 .
[12] FIRST HIGH CONTRAST IMAGING USING A GAUSSIAN APERTURE PUPIL MASK , 2002, astro-ph/0205123.
[13] David Mouillet,et al. NAOS, the first AO system of the VLT: on-sky performance , 2003, SPIE Astronomical Telescopes + Instrumentation.
[14] High-contrast coronagraphy with NGST in the mid-IR , 2003 .
[15] Anthony Boccaletti,et al. The Four‐Quadrant Phase Mask Coronagraph. III. Laboratory Performance , 2003 .
[16] "Planet Finder" on the VLT: context, goals and critical specifications for adaptive optics , 2003 .
[17] F. Wildi,et al. Adaptive Optics Nulling Interferometric Constraints on the Mid-Infrared Exozodiacal Dust Emission around Vega , 2004, astro-ph/0406587.
[18] NACO Ks, Lp and M band imaging of NGC 1068 , 2004, Proceedings of the International Astronomical Union.
[19] David Mouillet,et al. Hot Very Small dust Grains in NGC 1068 seen in jet induced structures thanks to VLT/NACO adaptive optics , 2003, astro-ph/0312094.