TY - JOUR
T1 - High Contrast Imaging with the New Vortex Coronagraph on NACO
AU - Mawet, Dimitri
AU - Absil, Olivier
AU - Girard, Julien H
AU - Milli, Julien
AU - O’Neal, Jared
AU - Delacroix, Christian
AU - Baudoz, Pierre
AU - Boccaletti, Anthony
AU - Bourget, Pierre
AU - Christiaens, Valentin
AU - Forsberg, Pontus
AU - Gonté, Frederic
AU - Habraken, Serge
AU - Hanot, Charles
AU - Karlsson, Mikael
AU - Kasper, Markus
AU - Lagrange, Anne-Marie
AU - Lizon, Jean-Louis
AU - Muzic, Koraljka
AU - Peña, Eduardo
AU - Olivier, Richard
AU - Slusarenko, N.
AU - Tacconi-Garman, Lowell E
AU - Surdej, Jean
PY - 2013/6
Y1 - 2013/6
N2 - The installation and successful commissioning of an L'-band annular groove phase mask (AGPM) coronagraph on VLT/NACO is presented. The AGPM is a vector vortex coronagraph made from diamond sub-wavelength gratings tuned to the L'-band. The vector vortex coronagraph enables high-contrast imaging at very small inner working angles (here 0.09 arcseconds, the diffraction limit of the VLT at L'), potentially opening up a new parameter space in high-resolution imaging. During technical and science verification runs, we discovered a late-type companion at two beamwidths from an F0V star, and imaged the inner regions of β Pictoris down to the previously unexplored projected radius of 1.75 astronomical units. The circumstellar disc of β Pic was also resolved from 1 to 5 arcseconds. These results showcase the potential of the NACO L'-band AGPM over a wide range of spatial scales.
AB - The installation and successful commissioning of an L'-band annular groove phase mask (AGPM) coronagraph on VLT/NACO is presented. The AGPM is a vector vortex coronagraph made from diamond sub-wavelength gratings tuned to the L'-band. The vector vortex coronagraph enables high-contrast imaging at very small inner working angles (here 0.09 arcseconds, the diffraction limit of the VLT at L'), potentially opening up a new parameter space in high-resolution imaging. During technical and science verification runs, we discovered a late-type companion at two beamwidths from an F0V star, and imaged the inner regions of β Pictoris down to the previously unexplored projected radius of 1.75 astronomical units. The circumstellar disc of β Pic was also resolved from 1 to 5 arcseconds. These results showcase the potential of the NACO L'-band AGPM over a wide range of spatial scales.
M3 - Article
SN - 0722-6691
VL - 152
SP - 8
EP - 13
JO - The Messenger
JF - The Messenger
ER -