Coronagraph: The design of the apodized prolate Lyot coronagraph (APLC) is developed in a series of papers by Remi Soummer et al., starting with Soummer et al. 2003 and 2005. Specifically GPI implements a set of achromatic optimized apodization functions as described in Soummer et al. 2011.
An APLC has optical elements in three planes:
Each GPI coronagraph consists of a matched set of apodizer+FPM+Lyot mask.
Masking of Nonfunctional Actuators:
Nonfunctional actuators in the MEMS tweeter deformable mirror must be masked out in the Lyot plane or else they will diffract additional light into the final image. To do this, there are opaque tabs included in the Lyot mask design.
There are four nonfunctional actuators on the MEMS DM used as GPI’s “tweeter” mirror (device serial number 080, which shows up in the Lyot mask part names.). In a coordinate system such that the center of the primary is located at (x,y) = (35.5, 32.5), the nonfunctional actuators are (53, 41), (24, 49), (47, 15), and (27, 27). In addition there is a pair of adjacent actuators that are not dead but are coupled together, at (40, 27) and (40, 28).
Astrometric Satellite Spot Grid:
The geometry of the Gemini South primary is one of the boundary conditions for GPI’s coronagraph. The pupil stop is the secondary mirror, M2, which is undersized relative to the primary to minimize the thermal background (and to allow for chopping in mid-infrared observations, though that’s no longer done). In the case of Gemini South the M2 is further stopped down by an opaque mask that baffles a slight turned-down region at the outer edge of M2. Also M2 has a hole through its middle which prevents directretroreflection of thermal emission back to the instruments.
Outer Diameter: 7.7701 m (projected diameter of baffle on M2)
Inner Diameter: 1.2968 m (projected diameter of M2 inner hole)
Secondary Supports: The secondary supports are only 1 cm wide, except for the one with the laser launch feed which is 1.4 cm wide. They are not an orthogonal cross, but rather are a pair of Vs, each 93.8 degrees wide with vertices offset from the primary center by 0.2179 m.
Because the Gemini telescopes were optimized for the thermal infrared, the secondary supports are very thin compared to most telescopes, and have correspondingly little effect on the PSF. However we mask them out in the Lyot planes regardless.
The GPI apodizers are fabricated using microdot printing. See Sivaramakrishnan et al. 2009 for details of this technology and its characterization, and Sivaramakrishnan et al. 2010 for for fabrication details and images of masks.
Name Outer Diameter
The focal plane masks are implemented as highly precise circular holes in mirrors. The same FPM is used for both K1 and K2. These masks were fabricated using deep reactive ion etching in gold-coated silicon mirrors. See Sivaramakrishnan et al. 2010 for fabrication details and images of hardware.
|Name||Diameter (mas)||Diameter (lambda/D)|
|Y||156.2||5.6 for Y|
|J||184.7||5.6 for J|
|H||246.7||5.6 for H|
|K1||246.7||5.6 for K1, 5.08 for K2|
There is also a mirror with no occulter hole, which sends the entire field of view to the IFS. THis is used for direct and NRM observations. For obscure historical reasons  this mask is labeled as the ‘SCIENCE’ position in the
The selected focal plane mask is recorded in FITS keyword OCCULTER, using variable names with Gemini-style name formatting, e.g. FPM_H_G6225 instead of just H.
The Lyot masks are named starting with the string ‘080m12’. This refers to the specific MEMS DM used for GPI (serial number #80), and the mask version modified in 2012.
The below table gives the mask geometries as they appear projected (rescaled) onto the primary mirror. The actual physical parts are just under 1 cm in diameter.
|Mask Name||Outer Diam. (m)||Inner Diam. (m)||Support Width (m)||Bad Act. Mask Diam.||Notes|
The 080_04 mask is an older generation and only has 3 bad actuators masked. The 080m12_04_c mask is a variant of 080m12_04 that has an additional 5th tab to mask out the two coupled actuators near the projected M2.
|||Because it sends all the light to the science camera.|